The galaxy presents a primarily smooth morphology, with a notable lack of distinct spiral arm structures or prominent dust lanes visible at this resolution. The overall shape is elliptical, appearing elongated or cigar-shaped rather than perfectly spherical. There is a concentration of light towards the center, suggesting a prominent galactic bulge. The color gradient transitions from a bluer hue at the outer edges to a redder tone in the central region, potentially indicating a younger stellar population in the outer regions and older stars concentrated in the core. There appear to be no significant signs of ongoing major merger activity or tidal disruptions. Minor disturbances cannot be ruled out.
