The galaxy appears as an elliptical or lenticular type, displaying a relatively smooth light distribution without prominent spiral arms or bar structures. Its shape is moderately elongated, tending towards a less circular form. A bright, concentrated central bulge is evident, indicating a high density of stars toward the galaxy's core. The outer regions of the galaxy exhibit a gradual decrease in luminosity, forming an extended halo. The color profile suggests a population of older stars. It seems to exhibit ongoing, low-level star formation. There is no obvious evidence of a major ongoing merger.
