The galaxy presents as an elongated, cigar-shaped structure with a smooth, diffuse appearance. The central region exhibits a yellowish hue, suggesting an older stellar population. The outer regions display a bluer tint, possibly indicating the presence of younger stars or ongoing star formation, though overall star formation is likely subdued. There is no apparent spiral structure or prominent dust lanes visible. There is no clear evidence of a major merger event, though slight asymmetries or minor disturbances cannot be ruled out. Overall, the galaxy appears to be a relatively massive, evolved system.
