The galaxy presents as a centrally concentrated mass of older stars, displaying a yellowish-white hue that suggests an evolved stellar population. Its overall structure is somewhat elongated, exhibiting a slight cigar shape, though possessing an ellipticity that is not extreme. There is no readily discernible structure or disk component. The smooth, blended light profile supports a classification as an elliptical galaxy, or possibly a lenticular galaxy viewed at an angle. No active galactic nucleus or star formation is clearly visible in the image. Based on its color, morphology, and estimated distance, this galaxy appears to be a relatively massive system, exhibiting minimal ongoing star formation. There are no obvious signs of any recent merger activity.
