The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slight ellipticity, appearing more elongated than perfectly circular. The central region displays a yellowish-orange hue, possibly indicative of an older stellar population. Moving outward from the core, the color transitions to a bluer tone in the surrounding regions, suggesting the presence of younger, hotter stars. No distinct spiral arms or bar structures are discernible. There is no obvious sign of any major ongoing merger activity or significant tidal disturbances. Faint extensions or halos may be present, but the resolution is insufficient to clearly define such features. The overall impression is of a relatively quiescent galaxy with a dominant bulge component and a less prominent, bluer disk.
