The galaxy appears as a somewhat elliptical object with a smooth, concentrated light distribution. There is a subtle color gradient, transitioning from a slightly bluer hue in the central region to a redder hue in the outer regions. No distinct spiral arms or prominent dust lanes are discernible. The overall morphology suggests a relatively evolved system, potentially a lenticular or elliptical galaxy. The relative lack of blue light suggests a lower rate of on-going star formation, with the redder colors hinting at an older stellar population dominating the light output, more apparent on the edges. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or recent mergers.