The galaxy presents as a centrally concentrated object, likely an elliptical or lenticular galaxy given its overall smooth appearance. The central region is notably brighter and exhibits a yellowish-white hue, indicating a significant population of older stars. The galaxy’s profile gradually fades outwards from the core with a redder tone, suggesting a radial color gradient possibly due to differential stellar populations or dust absorption. There is very little evidence of spiral arms or significant dust lanes. There might be a very faint disc structure. The light is overall consistent and does not have significant star formation. The morphology suggests that the galaxy is relatively isolated, undisturbed, and not currently undergoing any major merger events. The shape appears to be somewhere between round and oblong.
