The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge region that appears yellowish-orange, indicative of an older stellar population. The light gradually fades towards the outer edges. There is a slight elongation, however, it remains relatively rounded overall. The galaxy appears largely undisturbed. No major tidal features or signs of ongoing mergers are immediately apparent. Subtle color variations are observed across the galaxy, with a hint of bluer tones in the outer regions compared to the redder core, potentially suggesting ongoing star formation although at a low rate. The galaxy is relatively compact, with a moderate angular size.