The galaxy presents as a relatively smooth and centrally concentrated object, exhibiting a morphology consistent with an early-type galaxy, likely an elliptical or lenticular type. The light distribution is dominated by a prominent bulge, appearing almost spherical, with a gradual falloff in surface brightness toward the outer regions. There is a suggestion of slight elongation or asymmetry, but no distinct spiral arm structures or significant dust lanes are discernible. The core of the galaxy appears yellowish-orange, indicative of an older stellar population. Fainter, bluer hues are observed in the outer regions of the galaxy. Overall, there is a subtle hint of a disk-like structure, but no clear indication of ongoing star formation. No signs of any major merging events or tidal disturbances are evident in the morphology of the galaxy.
