The galaxy appears as a single, largely uniform object with a generally elliptical morphology. The galaxy presents with a smooth profile, suggesting a lack of significant spiral arm structure or prominent dust lanes. There is no indication of ongoing merging activity or significant tidal disturbances. A slight color gradient is observed, with the central region exhibiting a more yellowish or reddish hue, potentially indicating an older stellar population concentrated in the bulge. The outer regions appear somewhat bluer, which might imply the presence of some younger, hotter stars. However, the overall color is relatively red, suggesting a population dominated by older stars. There is no strong evidence of active star formation. The galaxy's round shape is indicative of it being primarily an elliptical galaxy with little rotation.
