The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a soft, ellipsoidal morphology, appearing more in between round and cigar-shaped than a defined disk or sphere. The color profile reveals a dominant yellowish-white hue in the central region, indicative of an older stellar population and lower levels of ongoing star formation. The outer regions show a very faint blue tint, suggesting a small population of younger, bluer stars possibly in sparse and loosely organized spiral features or regions of more recent star formation. There is no strong evidence of significant tidal distortions or major merging events; the galaxy appears largely undisturbed. The central bulge appears more prominent than any surrounding disk, but this may be due to the viewing angle and light integration along the line of sight. The galaxy lacks the distinct, sharply defined features typically associated with actively star-forming spiral arms or pronounced dust lanes. Overall, the galaxy's morphology is consistent with that of an early-type spiral or a lenticular galaxy approaching a more quiescent state.
