The galaxy presents as a relatively compact object. Its morphology appears primarily smooth, with a slightly elliptical shape, closer to in between round and cigar shaped. There is no clear evidence of spiral arm structure or a prominent central bulge. The color profile suggests the presence of older stellar populations, with a redder hue dominating its overall appearance. There is no obvious active galactic nucleus. There appears to be only minor disturbances of the object, which otherwise looks like an isolated galaxy. The galaxy's luminosity falls within a moderate range, indicating a likely intermediate stellar mass. Star formation activity is estimated to be relatively low, with a very low specific star formation rate.
