The galaxy presents as a largely featureless, elliptical structure with a concentrated central bulge. The light profile suggests a relatively smooth distribution of stars. The galaxy appears almost spheroidal. There is little evidence of spiral arms or dust lanes, although the image quality is limited. Color suggests an aging stellar population, with a redder hue indicative of older, less massive stars dominating the overall light output. Star formation rate appears to be relatively low based on the lack of blue light, associated with younger, more massive stars. The galaxy shows no apparent signs of recent or ongoing major merger activity, appearing isolated and undisturbed. There may be some minor disturbances but it is unclear.