The galaxy presents as a relatively smooth, elongated structure. Its dominant feature is a cigar-like shape, with a noticeable central bulge that appears slightly brighter and more concentrated than the outer regions. A faint disk is visible, with a bluish hue, suggesting the presence of younger, hotter stars and ongoing star formation, albeit at a moderate rate. There are no clear signs of spiral arm structure or prominent dust lanes, giving the galaxy a generally featureless appearance. Indications suggest a galaxy with an intermediate mass. There is no evidence of ongoing major mergers, although minor tidal disturbances cannot be ruled out. Overall, the galaxy appears to be a well-defined, disk-like system with a prominent bulge and some degree of ongoing star formation.
