The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated luminosity profile with a gradual decrease in surface brightness outward. The galaxy's overall shape is closer to round than elongated, though it is slightly elliptical. There is a subtle hint of minor disturbances in the outer regions, but the overall structure is not heavily disrupted. The primary color of the galaxy is a warm hue, suggesting a population of older stars. There is a hint of bluer light in the central region, possibly indicating recent, localized star formation. The galaxy lacks prominent spiral arms or a well-defined disk structure. No obvious signs of a major merger are present, although there is a possibility of minor interactions with smaller galaxies.
