The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable central bulge. It appears to be a fairly rounded system with a somewhat diffuse outer halo. The color gradient suggests a redder core, possibly indicative of an older stellar population concentrated in the bulge, gradually transitioning to bluer hues in the outer regions. This color distribution could indicate ongoing, albeit low, levels of star formation in the outskirts. Faint disturbances in the outer disk can be noted. The galaxy appears to be relatively isolated, with no obvious signs of major tidal interactions or mergers in progress.
