The galaxy appears as a relatively smooth, centrally concentrated object. Its overall morphology is elliptical, presenting an elongated but not strongly cigar-shaped form. There's a slight indication of a central bulge, although it's not sharply defined. No distinct spiral arms or bar structures are discernible. The galaxy's light distribution appears relatively uniform, suggesting a lack of significant recent star formation. There's no evidence of strong tidal features or major disturbances suggestive of ongoing merger activity, although a subtle asymmetry might hint at a minor interaction. The galaxy exhibits a yellowish-white hue, indicating a population of older stars with minimal dust obscuration. The galaxy's apparent size is small but detectable.
