The galaxy presents an elongated, cigar-shaped morphology. It exhibits a smooth, diffuse appearance across its entire structure, lacking any distinct spiral arms or other prominent features. The light distribution is generally concentrated toward the center, gradually fading towards the outer edges. A subtle color gradient can be observed, with the central regions appearing slightly more yellow-red and the outer regions possessing a blue tint, possibly indicating differing stellar populations or dust distribution. No signs of active galactic nuclei or major disturbances, such as tidal tails or merging activity, are evident within the limits of the data. Overall, the galaxy appears to be an undisturbed, elliptical system.
