The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentrated central bulge that appears nearly spheroidal. The light distribution suggests a gradual decrease in intensity from the core outwards, with no apparent spiral arm structure or prominent dust lanes visible in this imaging. There's a slight elongation in its overall shape, verging towards a mild cigar-shape morphology. The galaxy displays a color gradient, with a reddish hue concentrated at the center which shifts to a greener color towards the outer edges of the galaxy. The colors indicate the likelihood of an aging stellar population, although star formation is possible at a low rate. The galaxy appears relatively isolated, showing no signs of ongoing major merger activity or tidal disturbances.
