The galaxy presents an overall smooth and relatively featureless appearance. Its morphology appears to be elliptical, elongated in shape, and cigar-like. The color gradient observed transitions from a bluer hue on the outer edges toward a more yellowish-red core, indicating a potential gradient in stellar populations, with younger, bluer stars perhaps populating the outer regions and older, redder stars concentrated towards the center. There are no prominent spiral arms or dust lanes visible. There is no obvious sign of any major mergers or tidal disturbance.
