The galaxy presents as a slightly elliptical, diffuse object. A central bulge is visible, exhibiting a yellowish hue, suggesting a population of older stars. The outer regions of the galaxy show a bluer tint, indicative of ongoing star formation. There are no distinct spiral arms or bar structures readily apparent, but there is a general disk-like structure with some minor disturbances visible. The overall appearance is somewhat smooth, but not entirely featureless, suggesting either a later-type spiral galaxy with faint arms, or an early type galaxy. There is no evidence of a major merger event, however, there are some faint, minor irregularities that might indicate a smaller gravitational interaction. The galaxy displays moderate levels of star formation.
