The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. The core is bright and displays a yellowish hue, potentially indicating an older stellar population. There's minimal evidence of spiral arms or distinct features beyond the central bulge; the light distribution fades gradually outwards with a more reddish tint, suggesting a spheroidal morphology. There does not seem to be any active galactic nuclei that would be very bright at the center. No obvious signs of ongoing major mergers or tidal disturbances are visible in the galaxy's immediate vicinity.
