This galaxy presents an elliptical morphology, exhibiting a smooth, concentrated central bulge that graduates outwards to a fainter, diffuse halo. The object has a noticeable elongation, with the major axis extending approximately three times the length of the minor axis. There is a gradual color gradient from the inner to the outer regions, trending from a yellow-red hue in the core towards a greenish tint in the periphery. This suggests that the galaxy is populated by older stars in the central bulge, while star formation may be occurring in the outer regions. There is no evidence of spiral arms, bars, or tidal disturbances. The overall structure seems to be undisturbed, indicating that it is likely not undergoing any major merger events.
