The galaxy presents a predominantly smooth morphology, with a central bulge that appears almost spheroidal. The color profile indicates a relatively evolved stellar population, with a yellowish-white core transitioning to bluer hues in the outer regions. This color gradient suggests ongoing or recent star formation activity, particularly within what may be a faint, disk-like component extending from the central bulge. There are some minor irregularities in the outer regions of the disk, possibly indicating tidal interactions or minor mergers. The overall shape is tending towards round rather than cigar-shaped.
