The galaxy appears to be a lenticular or early-type spiral galaxy, with a generally smooth appearance and elongated shape. The central bulge is bright and dominates the galaxy's luminosity, exhibiting a yellowish-orange hue indicative of an older stellar population. There is little visible dust or distinct spiral arm structure, suggesting a relatively quiescent star formation history. The galaxy displays an overall cigar-like morphology, with a gradual decrease in surface brightness from the core outwards. There's a slight asymmetry in the outer regions, hinting at potential tidal interactions or minor disturbances, but the galaxy appears largely undisturbed. The lack of prominent features suggests that this is likely a mature galaxy, potentially transitioning away from active star formation.
