The galaxy presents as a relatively compact, somewhat irregular structure. A central, diffuse bulge is observed with a slightly elongated, disk-like component extending outwards. The dominant color is a subtle yellow-white, suggesting an older stellar population in the bulge. A bluer, patchy region is observable on one side of the galaxy, which could indicate regions of more recent star formation. There appears to be some disturbance within the galaxy, possibly caused by an interaction or merger. There is no strong evidence of spiral arms; the overall appearance is more indicative of a galaxy undergoing a dynamic evolutionary process.
