The galaxy presents as a moderately elongated, disk-like structure. The central bulge appears bright and concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. The disk component shows a smoother texture with a subtle blueish tint, possibly indicating areas of recent or ongoing star formation, although at a suppressed rate. The galaxy exhibits a minor disturbance in morphology, but is not undergoing a major merger. Overall the galaxy appears relatively isolated and undisturbed. The galaxy is a smooth, elliptical object.
