The galaxy presents a largely smooth and rounded morphology, suggesting a classification leaning towards elliptical. There's a notable concentration of light towards the center, indicative of a prominent galactic nucleus. The color profile suggests a moderate population of older stars, potentially exhibiting a redder hue in the central regions. While the overall structure is smooth, there's a hint of irregularity in the outer regions, but it is still mainly smooth. There is no apparent spiral structure or disk, and minimal evidence of ongoing major mergers or significant tidal disturbances. The estimated size suggests it's a relatively large galaxy.
