The galaxy presents a generally smooth, elliptical morphology. It appears to be quite massive, exhibiting a centrally concentrated, bright core that gradually diffuses outwards. The color is predominantly yellow, suggesting an older stellar population with less active star formation. There is a slight elongation, deviating from a perfectly circular form, with a hint of a possible minor disturbance or tidal feature. These slight disturbances could also point to possible recent mergers. This suggests that the galaxy has undergone, or is currently undergoing, some type of gravitational interaction. Star formation rate appears to be relatively low.
