The galaxy presents as a somewhat elliptical, relatively featureless object. The core region exhibits a concentrated, bright, yellowish-white luminosity, suggesting an older stellar population. Moving outward from the core, the light gradually diminishes in intensity. A faint, diffuse halo surrounds the core, displaying a subtle blueish tint, possibly indicating some ongoing star formation, though at a low rate. The overall smooth appearance and color gradient are consistent with an early-type galaxy, likely an elliptical or lenticular type. There is a slight elongation, suggesting the galaxy is not perfectly spherical, but rather somewhat flattened. No distinct spiral arms or dust lanes are readily apparent within the resolution of the image. The galaxy appears relatively isolated, showing no obvious signs of recent major mergers or tidal interactions.
