The galaxy presents as an elliptical morphology. It exhibits a notably elongated, cigar-like shape. The galaxy's color profile suggests a dominant population of older stars, with a reddish hue concentrated towards the central bulge. Fainter blue-ish colors are visible near the edges of the disk. There is no spiral arm structure that is immediately apparent. There are no signs of significant disturbances suggesting that it is not currently undergoing a major merging event, although there may be some minor perturbation. The luminosity is very high.
