The galaxy presents as a resolved object with a generally elliptical morphology. The central region appears to be dominated by older stellar populations, exhibiting a yellowish-orange hue. Evident within the galaxy are regions displaying bluer colors, suggestive of active star formation. These areas appear somewhat patchy and are distributed non-uniformly across the galaxy's disk, giving the galaxy a slightly disturbed appearance. There is evidence of potential tidal features or minor irregularities in the galaxy's outer regions, which could be indicative of past or ongoing interaction with a companion galaxy, or potentially an internal disruption.
