This galaxy presents as a relatively compact object with a dominant central bulge. The morphology appears intermediate between elliptical and spiral, with a suggestion of a flattened disk component, though distinct spiral arms are not readily discernible. The light distribution is centrally concentrated, with a smooth gradient outwards.

The color profile suggests a predominantly older stellar population, with the blue hue indicating some ongoing star formation, particularly towards the center. There is a slight asymmetry in the outer regions, possibly indicative of tidal interactions or minor disturbances, although no clear evidence of a major merger is apparent.
