The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The color profile indicates an older stellar population, showing a reddish hue in the central bulge and a slightly bluer, though still relatively muted, disk. There are subtle features suggesting some degree of rotational symmetry. Based on the slight irregularities in the outer regions, it is likely the galaxy is not completely undisturbed; there might be some tidal features suggesting possible past interactions or minor disturbances. Star formation appears to be present but relatively low, consistent with its overall redder colors. The galaxy is mostly round in shape, with very little, if any, distortion.
