The galaxy presents a complex morphology, suggestive of an ongoing or recent interaction. The primary body of the galaxy appears relatively smooth and elliptical, with a concentrated central bulge exhibiting a yellowish hue. This indicates an older stellar population dominating this region. Extending from this central region, there appears to be two distinct, brighter knots. The lower one shows a more diffuse structure, with a less defined boundary. There are some irregular features and faint tidal-like extensions that may be indicative of gravitational disturbances. The overall shape appears somewhat rounded. The color index suggests the presence of both older and possibly younger stellar populations contributing to its observed luminosity. There appears to be some disruption in the structure, possibly from an ongoing merger.
