The galaxy presents as a moderately luminous object with an overall elliptical morphology. It displays a smooth, diffuse light distribution, with a centrally concentrated bulge exhibiting a yellowish hue. This suggests a population of older stars within the bulge. The outer regions of the galaxy appear less concentrated, with a fainter, bluer color gradient suggesting the presence of some younger stars or ongoing star formation in the disk component. There is little evidence of strong spiral arm structure or prominent dust lanes. The overall impression is of a relatively undisturbed system, likely a galaxy that has undergone significant internal evolution. There is a slight tidal stream that is barely visible on the left side of the galaxy, indicating some past interaction with another galaxy.
