The galaxy presents as an elongated, cigar-shaped structure, with a color gradient suggesting a possible age stratification across its body. The central region appears diffuse and relatively brighter, potentially indicating a higher stellar density. The galaxy's color appears to shift toward redder hues towards the poles of its major axis. Irregularities are visible within the structure, possibly indicating mild gravitational interactions or internal disturbances. A lack of strong spiral arm structure, and the smooth appearance, are consistent with a classification toward the elliptical end of the galaxy morphology spectrum, but with faint features. 