The galaxy presents as a singular, centrally concentrated light source. The object has a generally smooth appearance, with no obvious spiral arm structures or significant dust lanes visible in the image. The light is yellowish-white in color. The overall morphology appears to be elliptical, exhibiting a high degree of roundness. There is no clear indication of tidal tails, merging companions, or major disturbances in its form. The surrounding field does not show evidence of ongoing interaction or recent merger events involving this galaxy. The stellar population appears to be largely composed of older stars, consistent with the observed color.
