The galaxy presents as a relatively small, lenticular-shaped object. Its central bulge appears smooth and featureless, exhibiting a concentrated luminosity profile. A faint, extended disk is discernible, although its structure lacks prominent spiral arms. The galaxy displays a bluish tinge, which could indicate ongoing, but relatively low, star formation activity within the disk. There is a slight asymmetry to the galaxy's overall shape, with one side of the disk appearing more extended or disturbed than the other. This could be indicative of a minor gravitational interaction with a nearby object, or a recent accretion event. Overall, the galaxy appears to be an intermediate mass object, potentially transitioning from a more actively star-forming spiral to a quiescent elliptical. There is no visual evidence of a major ongoing merger, although the possibility of past interactions influencing its current morphology cannot be ruled out.
