The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. The core region exhibits a yellowish hue, suggestive of an older stellar population. A subtle, elongated structure is visible, indicating it is not perfectly spherical. There are hints of a diffuse, bluish disk component surrounding the central bulge, possibly indicating a low level of star formation activity. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances. Overall, it appears to be a relatively quiescent galaxy.
