The galaxy presents a generally smooth morphology, with a concentrated central bulge. The overall shape is somewhat elliptical but leans toward being in between elliptical and round. There are no clearly defined spiral arms or a distinct disk. There is a very slight suggestion of asymmetry, which may indicate a minor gravitational disturbance, but this is subtle. The light profile appears to be centrally concentrated. The color suggests a dominant older stellar population, with a redder hue, particularly in the central regions. There is little evidence of recent or ongoing major star formation. The estimated size is approximately 7 kpc, suggesting a fairly compact but not dwarf-sized system.
