This galaxy presents as a centrally concentrated, elliptical-like structure. The core region exhibits a yellowish-orange hue, indicative of an older stellar population. Moving outwards from the core, the color shifts to a bluer tone, suggesting the presence of younger, hotter stars in the galaxy's outer regions. The galaxy appears relatively smooth and symmetrical, without any obvious spiral arms or strong irregularities. There is a slight asymmetry in the distribution of the bluer light. The galaxy is relatively compact. The overall morphology suggests a galaxy that is, or has undergone, a transition toward a spheroidal shape, with limited ongoing star formation within the nucleus and a greater presence of younger stars in the surrounding regions. Evidence suggests that this galaxy is not currently undergoing any major merger activity, as it appears undisturbed. However, very minor disturbances cannot be fully ruled out.
