The galaxy appears as a single, relatively smooth object with a concentrated central bulge. Its shape is approximately round, exhibiting a generally elliptical morphology. The light distribution suggests an older stellar population, with a yellowish-red hue dominating the galaxy's emission, although there are hints of bluer regions, possibly indicating some on-going star formation, but at a low rate. There's no readily apparent spiral structure, but a subtle disk-like component cannot be ruled out. The galaxy does not appear to be undergoing a major merger, although there is a possible slight distortion in its overall shape, implying a recent or on-going minor gravitational interaction. The size is relatively compact, spanning approximately 6.7 kpc.
