The galaxy presents a concentrated central bulge, appearing largely spheroid with a smooth light distribution. The core region exhibits a yellowish-orange hue, indicative of an older stellar population. There are small hints of disturbed morphology, with a slight asymmetry in the outer light distribution. There is evidence of a faint red region located above the core, indicating potential recent or ongoing star formation in that area. Overall, the galaxy seems to have an elliptical morphology with a relatively high mass and very little to no star formation. The diameter measures roughly 12 kpc. There also appears to be signs of merger activity.
