The galaxy presents a somewhat lenticular morphology, appearing largely smooth with a subtle disk-like structure. The nucleus exhibits a moderate concentration of light, while the overall color profile suggests an intermediate stellar population, with a hint of ongoing or recent star formation.

There are indications of minor disturbances or interactions within the galaxy. The overall structure appears asymmetrical, possibly hinting at a past merger event or ongoing tidal interactions. The presence of bluer regions implies the likelihood of pockets of active star formation.

The estimated size of the galaxy, spanning roughly 4 kiloparsecs, places it within the realm of dwarf or intermediate-sized galaxies. Its absolute magnitude suggests it is a reasonably luminous galaxy, despite its relatively small size. Overall, this galaxy presents itself as a dynamic object, likely undergoing evolutionary processes driven by internal activity and external interactions.
