The galaxy presents a generally smooth morphology, appearing as a single, concentrated object with a somewhat diffuse edge. It exhibits a slight elongation, appearing somewhat between round and elliptical. There is a suggestion of asymmetry, with some possible minor disturbances in its overall shape.

The galaxy's color gradient indicates an older stellar population with a relatively redder hue in the central regions, gradually transitioning to a bluer tint in the outer areas. This may suggest a difference in stellar ages and metallicities between the core and the outer regions.

There is a hint of a faint, extended halo surrounding the central region, although it's difficult to determine the exact extent and structure of this halo without further data. Based on the somewhat disrupted shape and the colour variation, there could be a possible minor merger with a smaller companion.
