The galaxy presents an elliptical morphology. It has a bright, concentrated central bulge that is surrounded by a more diffuse halo. The color profile suggests older stellar populations within the bulge, indicated by the presence of redder hues. The outer regions of the galaxy display a subtle bluer tint, potentially suggestive of some younger stars or ongoing, though limited, star formation. There is no visible spiral arm structure or bar feature, and the galaxy shows a high degree of symmetry. Overall, the galaxy appears to be a relatively quiescent system with evidence of some limited star formation activity in its outer regions. No major signs of tidal disturbances or interactions are apparent, but there might be some minor irregularities.
