The galaxy presents a generally elliptical morphology, appearing more elongated than spherical. The central region exhibits a concentrated, bright bulge. Moving outwards from the core, the light appears to fade gradually, with no sharp edges or distinct spiral arm structures immediately apparent. There is a slight asymmetry in the outer regions, suggesting potential past interactions or minor disturbances. The colour profile indicates a yellow-red hue in the central bulge, possibly indicating an older stellar population, while the outer regions display a slightly bluer tint, which may signify the presence of younger stars or ongoing star formation. Overall, it seems to be a disk galaxy that is moderately evolved with some disturbance due to a merger in its past.
