The galaxy appears to be a relatively smooth, elliptical type. The overall shape is elongated, exhibiting a cigar-like appearance. The central bulge is bright and concentrated, displaying a yellowish hue, suggesting an older stellar population. The outer regions show a gradual decline in luminosity, with a subtle color gradient towards bluer tones, potentially indicating some ongoing star formation, albeit at a low rate. There is no evidence of spiral arms or significant dust lanes within the visible spectrum. The overall morphology indicates a galaxy that has likely undergone significant evolutionary processes, potentially including mergers or interactions in the past, which has led to its currently relaxed, elliptical form. There is a slight asymmetry observed, possibly indicating some minor past interactions.
