The galaxy presents as a moderately bright, relatively smooth object, potentially an elliptical galaxy or a lenticular type galaxy. It appears to be largely featureless, lacking the spiral arm structures characteristic of spiral galaxies. The light distribution suggests a centrally concentrated spheroid with a gradual decline in brightness towards the edges. There is a slight suggestion of bluer light in the outer regions, which might indicate some ongoing, albeit subdued, star formation. The overall morphology is consistent with a system that has undergone substantial stellar evolution, possibly with an older stellar population dominating the light output. No signs of significant tidal interactions or merging events are readily apparent, although subtle disturbances may be present at a level below the image resolution. The shape appears generally round.
