The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth light distribution. There is a noticeable color gradient, shifting from a more yellowish-white core to redder hues towards the outer edges. The overall shape suggests a prolate spheroid, elongated along its major axis. No distinct spiral arms or dust lanes are visible, indicating a likely lack of significant ongoing star formation. There appears to be little or no evidence of tidal disturbances or interactions with other galaxies, suggesting it is an isolated system in a relatively quiescent state. The smooth morphology and color profile are consistent with an older stellar population.
