The galaxy presents as a relatively smooth, elliptical or spheroidal structure. The light profile exhibits a centrally concentrated bulge, gradually fading towards the outer regions. There is a lack of any discernible spiral arms or distinct features such as dust lanes within the galaxy's body, suggesting a lack of significant ongoing star formation. The color index appears redder, potentially indicating an older stellar population with minimal active star formation. No signs of tidal disturbances or mergers are apparent in the immediate vicinity. Based on its morphology, a classification as an elliptical galaxy is plausible.
