The galaxy appears as a moderately luminous, elliptical system with a smooth, centrally concentrated morphology. There is an absence of discernible spiral arms or a prominent disk structure. The galaxy exhibits a relatively regular, rounded shape with no obvious signs of significant tidal disturbances or ongoing major mergers, although minor disturbances cannot be ruled out. The color profile suggests a dominance of older stellar populations, indicated by the redder hues. The galaxy's overall appearance is consistent with a high probability of being a smooth galaxy with a round morphology. There is an absence of star-forming regions.
