The galaxy presents as a moderately sized, relatively smooth elliptical or lenticular system. It exhibits a concentrated central bulge, characterized by a yellowish-orange hue, indicative of an older stellar population. There is a subtle color gradient from the core outward, suggesting a gradual decrease in stellar age. The overall structure appears largely undisturbed, lacking any prominent spiral arms, dust lanes, or signs of recent major mergers. There are no obvious tidal tails or extended halos easily visible in this image.
