The galaxy presents as a mostly smooth, lenticular-like structure with a concentrated central bulge. There is evidence of a slight disk component, but it appears relatively featureless. The galaxy appears to be in isolation with no major disturbances or mergers. There are hints of tidal interactions, such as a potential stellar stream or disturbance in the outer halo, which could be the result of a minor interaction or flyby event. The colors suggest a stellar population dominated by older, redder stars. The overall morphology indicates a galaxy that is not actively forming many new stars, suggesting a relatively quiescent evolutionary state.
