This galaxy presents as a relatively smooth, elongated structure. The overall shape is cigar-like. The color gradient suggests a concentration of older stars towards the center, exhibiting a yellowish hue. The outer regions appear bluer, which could indicate the presence of younger, hotter stars and ongoing star formation. There is some hint of a disk-like feature. There is no strong evidence of a major ongoing merger or significant disturbance in the galaxy's morphology, although some minor asymmetries are present. Overall, the galaxy seems to be a fairly evolved system, with a mix of stellar populations and a generally smooth light distribution.
