The galaxy presents as a relatively compact object with a smooth, elliptical morphology. It exhibits a noticeable color gradient, shifting from a bluer hue in its central region to redder tones towards the periphery. This color gradient is suggestive of differing stellar populations, potentially indicating ongoing or recent star formation concentrated in the core, with an older, redder stellar population dominating the outer regions. There is potential evidence of a minor disturbance or interaction, given the slight asymmetry in the light distribution. No distinct spiral arms or a well-defined disk structure are visible. There is some evidence of a secondary body in the image that could represent an ongoing merger.