The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a concentrated, yellowish hue, suggesting a population of older stars. Moving outward from the core, a diffuse greenish-blue glow is observed, hinting at ongoing, albeit subdued, star formation in the outer regions. The overall shape is elongated, with a minor axis to major axis ratio that indicates a moderate degree of flattening. No distinct spiral arms or prominent dust lanes are discernible. The galaxy appears isolated, with no immediate signs of tidal disruption or interaction with neighboring galaxies.
