The galaxy presents a generally smooth morphology with a dominant central bulge. The bulge exhibits a concentrated luminosity profile. A fainter, more diffuse disk component is suspected, though the disk lacks distinct spiral arm features. The galaxy's overall shape appears to be somewhere between round and elliptical. There is a hint of a potential minor disturbance or interaction with a smaller, nearby object. This may be indicative of a past or ongoing merger event of some type. The galaxy exhibits colors suggesting moderate star formation activity.
