The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is little indication of spiral arm structure or significant dust lanes. The galaxy appears to be elongated, with a cigar-like shape. The central region exhibits a bright, concentrated core, surrounded by a more diffuse halo. The color profile suggests a population of older stars with a lower rate of star formation, transitioning from blue near the central bulge to red in the outer regions. There is no sign of a significant merger or major tidal disturbance. The galaxy appears undisturbed and relatively isolated.
