The galaxy exhibits a morphology that appears to be intermediate between elliptical and spiral. It presents a somewhat elongated shape, but it is not clearly disk-like. A notable feature is a bright, centrally concentrated bulge exhibiting a yellowish hue, suggestive of an older stellar population and reduced star formation. Moving outwards from the bulge, the galaxy transitions into a fainter, bluer region on one side. This bluer region could indicate more recent star formation activity compared to the central bulge. The overall light distribution suggests the galaxy is reasonably smooth, with only subtle irregularities in its form. There are slight indications of tidal tails.
