The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a spheroid-dominated morphology, exhibiting a gradual decrease in surface brightness from the core outwards. The core region presents a yellowish hue, potentially indicating an older stellar population. Fainter, reddish regions appear on the outer edges of the galaxy, possibly denoting areas of more recent, albeit subdued, star formation activity or dust obscuration. There are no distinct spiral arm features visible. Overall, the galaxy gives the impression of being a passively evolving system, with little evidence of significant ongoing mergers or major disturbances.
