The galaxy presents as a centrally concentrated object with a generally smooth morphology, suggesting an elliptical or lenticular classification. The light distribution appears to be fairly even, with a gradual decrease in intensity moving outward from the core. The shape is neither perfectly spherical nor highly elongated, appearing somewhat elliptical. There is no clear evidence of spiral arms, distinct dust lanes, or any major distortions indicative of recent mergers. The color profile suggests a population of older stars, as indicated by the subtle reddish hue.
