The galaxy presents as a fairly smooth, centrally concentrated object with a diffuse halo. The core region exhibits a bright, yellowish-white luminosity, suggesting an older stellar population. The surrounding halo appears more subtly colored with hints of blue and red, potentially indicating a mix of stellar ages. There is a slight elongation in the shape, deviating marginally from a perfect circular form; however, no distinct spiral arms or bar structures are discernible. No major signs of active galactic nuclei are immediately apparent, and there are only minor indications of disturbances or interactions with other galaxies. It appears to be a relatively isolated galaxy, with a morphology consistent with that of an elliptical galaxy.
