The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a yellowish hue, potentially indicating an older stellar population. A slight color gradient is noticeable moving outwards from the core, with the outer regions displaying a subtle greenish tinge. There does not appear to be any significant disk structure, or spiral arm morphology visible, suggesting the galaxy is an early-type morphology. The galaxy appears to be a fairly isolated system, with no apparent signs of tidal interactions or major disturbances to its shape. There is no evidence of any dust lanes or obscured regions. The overall appearance suggests a system dominated by an older stellar population, and a low star formation rate.
