The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth, featureless morphology. The light distribution suggests a spheroidal shape, being mostly round. A slight elongation is barely visible, with minimal deviation from a perfectly circular form. 

The galaxy exhibits a color gradient. The core displays a yellowish-red hue which then fades into a bluish halo as one moves away from the center of the galaxy. This color shift could reflect differences in the stellar populations, with older, redder stars dominating the central regions and younger, bluer stars contributing more to the outer regions. Based on the color, there is ongoing star formation at a modest rate. There are no obvious signs of spiral arms or a prominent disk structure. No signs of significant tidal disturbances or ongoing mergers are visible, which supports the overall smooth appearance.
