The galaxy presents a generally elliptical morphology, though not perfectly symmetrical. A central, bright nucleus is clearly visible, surrounded by a less luminous, more diffuse halo. The color appears to be primarily bluish-white in the central region, possibly indicative of a population of younger, hotter stars or active star formation. Extending outward from the center, the galaxy exhibits a subtle color gradient, transitioning toward a redder hue in the outer regions, which might signify an older stellar population. There is some slight patchiness in the galaxy's structure which may mean there are some weak spiral arms, or it is undergoing a minor disturbance with a merging companion. Overall, the galaxy appears relatively smooth, lacking prominent dust lanes or other distinct features.
