The object appears as a relatively smooth, centrally concentrated galaxy with a generally elliptical morphology. The light distribution is fairly uniform, suggesting a lack of strong spiral arm structures or prominent dust lanes. The dominant color is yellowish-orange, with a relatively tight concentration of the color in the center, possibly indicating an older stellar population or the presence of dust. There is no clear evidence of a significant ongoing merger event, though the color suggests low levels of star formation. Overall, the galaxy appears to be a moderately massive system, possibly a luminous early-type galaxy or a spiral seen face-on at a distance.
