The galaxy presents as a somewhat diffuse object with a centrally concentrated bulge. The central region exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Surrounding the core, there is a bluer, more diffuse halo, possibly indicative of ongoing or recent star formation within a disk-like structure. Irregularities in the outer regions of the disk suggest potential gravitational disturbances, possibly from a minor merger event or tidal interactions. There is some evidence of faint spiral arm structures, though these are not clearly defined. Overall, the galaxy exhibits characteristics of both an elliptical and a spiral galaxy, placing it somewhere along the morphological sequence, and suggesting possible transitional activity.
