The galaxy presents as a relatively small, well-defined object. Its morphology appears to be elliptical, showing a smooth, centralized distribution of light with no apparent spiral arm structure. The galaxy's light profile suggests a centrally concentrated bulge. There may be a very faint disk present. The color gradient across the galaxy is subtle, exhibiting a slightly redder hue in the central regions compared to the outer edges. No distinct signs of ongoing mergers or major disturbances are evident in the current image, though faint tidal features cannot be ruled out without deeper observations. Overall, it appears to be an isolated galaxy.
