This galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile with minimal discernible structure. The core region displays a yellowish hue, potentially indicating an older stellar population and reduced ongoing star formation. Moving outwards from the core, the color shifts towards a slightly bluer, albeit faint, tinge. This suggests a possible presence of younger, bluer stars in the outer regions, though their contribution to the overall luminosity is significantly less compared to the core. The galaxy lacks any obvious spiral arms or a prominent disk, supporting its classification as an elliptical. There is no clear indication of any significant tidal disturbances or ongoing merger activity, based on the smooth, undisturbed appearance of the outer halo. The galaxy is relatively compact, and the overall shape is nearly circular, though there is a subtle deviation from perfect roundness, suggesting it is somewhat elliptical.
