The galaxy presents a generally smooth and rounded morphology. The light distribution suggests an elliptical or lenticular classification, dominated by an older stellar population, as indicated by the overall yellowish hue. There is little evidence of spiral arms or significant dust lanes, further supporting a lack of ongoing, substantial star formation. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or recent mergers. Slight asymmetry may be present, potentially hinting at minor disturbances in the past, but the dominant impression is one of quiescence. The estimated size is on the order of several kiloparsecs.
