The galaxy presents a generally smooth morphology, with a concentrated central bulge. There is a subtle color gradient observable, transitioning from a yellowish-white core to a bluer, less concentrated outer region. No distinct spiral arms or bar features are apparent. The overall shape is approximately elliptical, appearing somewhat elongated, but predominantly spheroidal. There is no obvious indication of tidal features or ongoing major mergers, though a slight asymmetry in the outer regions could suggest a minor disturbance or past interaction. The galaxy's stellar population appears to be a mix of older, redder stars in the central region and younger, bluer stars in the outer regions, consistent with a system that has ongoing, but relatively low, star formation activity.
