The galaxy presents as a lenticular or possibly elliptical galaxy, with an elongated, cigar-like shape. The galaxy exhibits a smooth and concentrated light profile. The central region shows a high concentration of luminosity, with a gradual decrease in brightness towards the outer regions of the object. The color appears to be somewhat red, indicating a population of older stars, and suggesting a low rate of ongoing star formation. No distinct spiral arms or dust lanes are observable. The overall morphology suggests a relatively evolved galaxy with a bulge-dominated structure. The galaxy does not appear to be undergoing any major interactions or mergers.
