The galaxy presents as a centrally concentrated object with an elliptical morphology. There is a smooth, diffuse halo surrounding a brighter, more compact core. The galaxy exhibits a yellowish-white hue, indicative of an older stellar population. There is little evidence of prominent spiral arms or distinct dust lanes, suggesting a relatively quiescent star formation rate. The shape is neither perfectly spherical nor highly elongated, exhibiting a moderate ellipticity. Faint tidal features or minor disturbances may be present, but not strongly defined. The galaxy does not appear to be undergoing a major merger, but some interactions or minor disturbances cannot be ruled out.
