The galaxy appears as a flattened, elongated structure with a central bulge that is brighter and more concentrated. The morphology is suggestive of a disk galaxy viewed at an oblique angle. The overall color profile indicates a dominance of older stellar populations and a moderate rate of star formation. The galaxy's shape is decidedly cigar shaped, showing it to be elliptical in nature. There is no indication of ongoing major mergers or significant tidal disturbances. Subtle asymmetries may suggest minor interactions or internal processes are occurring, or they may be artifacts of observation. The light distribution appears relatively smooth, indicating a lack of prominent spiral arms or distinct star-forming regions. The color profile suggests a higher concentration of older stars towards the central bulge, which is typical of elliptical galaxies.
