This galaxy appears to be a relatively smooth, centrally concentrated object with a shape somewhere between elliptical and lenticular. There is a noticeable central bulge that is very bright and gradually fades into the galaxy's outer regions. The galaxy appears to be elongated, exhibiting a cigar-like shape, and there is little evidence of significant spiral arm structure or prominent dust lanes. There may be some subtle color variations across the galaxy, possibly indicating differences in stellar populations or star formation activity. The overall structure suggests a system undergoing relatively low levels of star formation, and it appears isolated, with no apparent signs of ongoing major mergers.