The observed galaxy presents a generally smooth morphology, appearing as an elliptical or lenticular type. There is a notable central bulge, characterized by a bright, concentrated luminosity, potentially indicating a high density of stars in the core. Surrounding the bulge is a fainter, more diffuse halo, with a slight disk-like appearance. The galaxy exhibits a blueish hue, concentrated towards the center. This color suggests the presence of relatively young stars, perhaps indicating a recent burst of star formation activity. The shape is mostly round, but does appear somewhat elongated. There is little evidence of spiral arms or significant dust lanes. No signs of tidal tails or other clear indications of ongoing mergers are visible, although there may be some minor irregularity present. The object's overall structure points towards an evolved system where much of the gas may have already been consumed, or where star formation is occurring at a relatively low rate.
