The galaxy presents as an elongated, cigar-shaped structure. It exhibits a relatively smooth morphology, with a dominant central bulge that appears yellowish in color, possibly indicating an older stellar population. Fainter blue regions extend from the central bulge suggesting the presence of younger, hotter stars and potential star formation occurring within these areas. The overall shape and smooth appearance suggest it could be an elliptical galaxy, although some evidence of a disk-like component may be present. There are subtle hints of a possible minor interaction or disturbance in the galaxy's structure.
