This galaxy appears to be a relatively smooth-featured system, likely a lenticular or early-type spiral. The shape is elongated, with a noticeable cigar-like morphology. It exhibits a central concentration of light, possibly indicative of a bulge component. Faint hints of disk-like structure are present, but without distinct spiral arms. There is a possible sign of minor disturbances or tidal features in the outer regions, but they are not indicative of a major merger. The overall color suggests a mix of stellar populations, with a dominant older population inferred from the redness, and a weaker component of ongoing star formation implied by bluer areas.
