The galaxy presents as a somewhat amorphous structure with a central, brighter region. It exhibits a generally blue hue, with hints of redder areas appearing on its periphery and in a concentrated area close to the central bulge. The overall shape appears disc-like but lacks defined spiral arms or a prominent bar. There are some visual distortions, but this could be a result of image artifacts. The galaxy is moderately compact and has a low to moderate estimated mass. Star formation appears subdued, with a low specific star formation rate. The light distribution suggests a mix of stellar populations, likely dominated by older stars. The galaxy shows signs of a past or ongoing minor merger.
