The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated morphology. It has a roughly circular shape, with a gradual decrease in luminosity from the core outwards. There is little to no evidence of spiral arms, dust lanes, or other features associated with disk galaxies. The color profile suggests a primarily older stellar population, with a yellowish hue dominating the galactic body, indicating a low rate of ongoing star formation. Faint irregularities are visible at the outer edges of the galaxy, suggesting the possibility of past interactions or minor disturbances. No obvious signs of a major merger event, such as tidal tails or strong asymmetries, are apparent. The galaxy presents as an isolated system with no directly interacting companions within the immediate vicinity.
