The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless structure with a high degree of roundness. It displays a concentrated central bulge that emits a strong, yellowish light, suggesting an older stellar population dominating the core. The light intensity gradually decreases from the center outwards, creating a diffuse halo. There is no evidence of spiral arms or significant dust lanes. Overall, it appears to be an isolated galaxy, not currently undergoing any major merging events or tidal disturbances.
