The galaxy presents as a relatively compact object. It exhibits a diffuse, unresolved structure with no discernible spiral arms or other distinct features. The overall color appears reddish, suggesting a population of older stars and/or significant dust obscuration. There is a possibility of a slight tidal disturbance or interaction, hinted by a subtle extension or asymmetry in its outer regions, though the resolution is insufficient to confirm this. The object lacks a clear nucleus or core, indicating a possibly spheroidal shape rather than a well-defined disk. The galaxy appears to be relatively isolated based on the surrounding field, with no obvious signs of an ongoing major merger.
