The galaxy appears as a slightly elongated, centrally concentrated object with a relatively smooth texture. Its color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue with a brighter core. There is little evidence of significant spiral arm structure or prominent dust lanes, which, along with the smooth appearance suggests a possible Elliptical Morphology. There is no obvious indication of major mergers or tidal disturbances in the immediate vicinity. The overall shape is neither perfectly spherical nor highly flattened but is more elliptical. Some minor asymmetry might be present, but it is not pronounced.
