The galaxy presents as an elongated, smooth structure, indicative of a likely elliptical morphology. The light distribution suggests a centrally concentrated spheroid with a gradual decline in surface brightness towards the outer regions. The core region exhibits a slightly redder hue compared to the outer halo, which appears somewhat bluer. This subtle color gradient may imply a differential distribution of stellar populations, with older, redder stars concentrated towards the core and younger, bluer stars more prevalent in the periphery. There is no visually discernible spiral arm structure or prominent dust lanes. Minor asymmetry, such as a slight tilt or warp, may be present. There does not seem to be signs of any major interactions or recent mergers, however, a slight warp could be indicative of a minor disturbance.