The galaxy presents as a generally smooth, elongated structure. It exhibits an elliptical morphology, appearing somewhat cigar-shaped. The core displays a higher surface brightness and a yellowish hue, suggesting a population of older stars. Moving outwards from the core, the galaxy gradually decreases in brightness and transitions to a slightly bluer color, hinting at the presence of younger stellar populations in the outer regions. There is no prominent spiral arm structure or bar visible. The overall impression is that of a relatively quiescent galaxy, possibly an early-type system. There is no obvious indication of ongoing major mergers or strong tidal disturbances, but subtle asymmetries might be present.
