The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, elliptical morphology with a bright central bulge. There's a subtle suggestion of a disk component without well-defined spiral arms, likely an Sa classification. The light profile indicates an older stellar population dominating, contributing to the overall redder hue.

The galaxy shows little evidence of active star formation, based on its color, suggesting a quiescent state. No signs of significant dust lanes or active star-forming regions are discernible. The overall structure does not reveal any major tidal disturbances or ongoing mergers, though there might be a hint of a minor interaction in the form of a slight asymmetry.
