The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a diffuse halo or envelope surrounding it. The color gradient suggests a redder central region, likely indicative of an older stellar population, while the outer regions may contain slightly bluer components, possibly hinting at some younger star formation. The galaxy appears elongated, deviating somewhat from a perfectly spherical shape. There are hints of minor structural disturbances, but no obvious major merging or tidal features are readily apparent. The galaxy's overall appearance indicates that it is a relatively massive system.
