The galaxy presents as a generally smooth object with a concentrated central bulge. The overall color profile leans towards redder wavelengths, indicative of an older stellar population, though some bluer regions are present, potentially suggesting ongoing or recent star formation activity. The galaxy exhibits a somewhat elliptical morphology, deviating moderately from a perfect circular shape. There may be some minor disturbances visible in the outer regions of the galaxy, but the overall structure appears relatively undisturbed. There is no clear evidence of a major merger event.
