The galaxy appears as a centrally concentrated, yellowish object. It exhibits a predominantly smooth morphology, with only subtle indications of internal structure. The overall shape is nearly circular, suggesting a minimal degree of apparent flattening. There is very little evidence of significant tidal disturbances or ongoing mergers. Based on the color, the galaxy may contain a significant population of older stars, and potentially be a moderate to high mass galaxy. Star formation appears to be relatively low.
