The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a generally elliptical morphology, appearing largely spheroidal in shape, with a slight deviation from perfect circularity. The luminosity profile appears to peak sharply in the center, suggesting a dense nucleus. The overall color is a yellowish-white, indicative of an older stellar population. There is little evidence of spiral arms, dust lanes, or significant star-forming regions. No signs of a recent or ongoing merger event are obviously present, though a slight asymmetry to the outer envelope is perceivable. The galaxy appears relatively isolated in this field of view.
