The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggestive of an older stellar population. There is faint evidence of a disk like structure that extends beyond the central bulge, displaying a subtle flattening. The galaxy appears to be experiencing some form of gravitational disturbance, evidenced by subtle asymmetries in its overall shape and the presence of faint tidal features extending outwards. The color indices indicate a higher concentration of older stars, giving it a redder overall hue, though some bluer regions are present, suggestive of some ongoing star formation. There is some evidence of a potential merging event, based on the irregularity of shape. Overall, the galaxy can be classified as an early-type galaxy with signs of recent or ongoing interaction with another galaxy.
