The galaxy presents an overall elliptical morphology. The central region exhibits a concentrated, bright core, indicative of a substantial stellar population. Moving outwards from the core, there's a relatively smooth transition in luminosity, though some faint, diffuse extensions are visible along the major axis. There is a slight flattening of the galaxy, but the overall shape is consistent with a spheroid. The galaxy appears relatively isolated, showing no signs of major tidal disturbances or interactions with other nearby galaxies. Color gradients suggest an older stellar population with a bias toward redder colors, possibly indicating lower levels of ongoing star formation. Based on these characteristics, it is likely a massive galaxy with a substantial mass.