The galaxy presents as a largely elliptical morphology, appearing generally smooth with no obvious spiral arm structures or significant dust lanes visible at this resolution. The central bulge exhibits a concentrated and relatively bright luminosity, suggesting a higher density of stars within that region. The color profile indicates a yellow-red hue dominating the central region, which could be indicative of an older stellar population. Moving outward from the center, there is a gradual shift towards a slightly bluer color, potentially suggesting the presence of a younger stellar population in the outer regions. Overall, the galaxy appears to be relatively isolated with no clear signs of recent major mergers or tidal interactions. Some minor disturbances may be present in the outer regions, but they do not significantly disrupt the galaxy's overall smooth structure. The object exhibits a near-spherical shape with only a slight deviation towards an elongated form.
