The galaxy presents a generally smooth, elongated morphology, suggesting a spheroidal or elliptical classification. It exhibits a color gradient, shifting from a concentrated yellowish-white core to a subtly bluish outer region along its major axis. The central region dominates the galaxy's overall luminosity. The elongated shape indicates a cigar-like appearance. There are no visible signs of spiral arms, significant dust lanes, or major disturbances. The smooth appearance is indicative of a galaxy that is undergoing few mergers. The change in color from the core to the extremities suggests a possible difference in stellar populations or ongoing star formation in the outer regions, although this is minimal. Overall, the galaxy appears to be a relatively quiescent system, possibly an early-type galaxy.
