The galaxy presents as a structured entity, with a generally elliptical morphology. The central region exhibits a concentrated luminosity, trending towards a yellowish hue, potentially indicating an older stellar population. A slight extension of the central region appears to be present, which could indicate the presence of a stellar bar. The outer regions of the galaxy display a fainter, more diffuse distribution of light, with subtle indications of ongoing or recent interaction. A region on the periphery shows hints of a more active star formation, as indicated by a faint blue-green color. The system displays some evidence of possible tidal disturbances or morphological asymmetry, possibly related to past or ongoing interactions or mergers. Overall, the galaxy appears to be a moderately luminous system.