The galaxy appears to be a relatively smooth, spheroidal structure, most likely an elliptical galaxy given its rounded shape and lack of prominent spiral arms. The core is bright and concentrated, with a noticeable decrease in luminosity as one moves towards the outer regions. The color gradient suggests an older stellar population, with a reddish hue dominating the central region. Faint blue-ish patches are present on its edges which could indicate some star forming activity, or potentially image artifacts. There is no clear evidence of ongoing major mergers, though there may be minor tidal disturbances in the periphery of the galaxy.
