The galaxy presents as an elongated, disk-like structure, displaying a relatively smooth appearance with a noticeable central bulge. The color profile suggests a significant population of older stars concentrated within the bulge, indicated by the yellowish-orange hue. The outer regions of the galaxy exhibit a bluer tint, possibly indicating the presence of younger stellar populations and ongoing star formation, even if not especially active. The galaxy's morphology appears to be intermediate between a spherical and cigar shape. There is a faint suggestion of minor disturbances in the galaxy's structure, hinting at past or ongoing gravitational interactions, but these are not prominently disruptive. The object's disk appears inclined relative to our line of sight.
