This galaxy presents as a centrally concentrated elliptical, exhibiting a smooth morphology with a lack of discernible spiral arms or distinct features. The core is characterized by a bright, yellowish-white hue, indicating a population of older, evolved stars. Progressing outwards from the center, the luminosity gradually decreases, and the color shifts towards a blue-green, potentially suggesting the presence of some younger stellar populations or a moderate amount of ongoing star formation activity. The outer regions are poorly defined, appearing somewhat diffuse and lacking sharp boundaries. There is no clear evidence of any major mergers or significant tidal disturbances in the immediate vicinity, though subtle asymmetries may suggest minor past interactions. Overall, the galaxy appears relatively quiescent.
