The galaxy presents as an elliptical or lenticular structure with a dominant, smooth morphology. Its central region exhibits a high concentration of light, suggesting a prominent bulge. The color profile indicates a generally redder hue overall, particularly towards the core, implying an older stellar population. There is a hint of a faint, bluer extension on one side, suggesting a possible, albeit minor, disturbance or a region of younger star formation. The galaxy appears relatively isolated with no obvious signs of ongoing major mergers, though minor disturbances cannot be ruled out completely. Its overall smooth appearance points towards a well-established, evolved system.
