The galaxy presents as a single, centrally concentrated object with a largely smooth morphology. There is little evidence of spiral arms or distinct substructure within the main body. The galaxy exhibits a generally elliptical shape. The light distribution appears relatively even, with a gradual decrease in intensity from the core to the outer edges. The galaxy has a noticeable yellowish hue, suggesting an older stellar population and potentially lower ongoing star formation activity. There are no signs of significant tidal disturbances or merging activity.
