The galaxy presents as a relatively smooth, elliptical morphology. The color profile suggests an older stellar population, with a dominant yellowish-orange hue in the central bulge region. The light appears more concentrated in the center and fades toward the edges of the galaxy, with the shape being akin to a cigar. There is no visible dust lane or distinct spiral arm structure. Overall, the galaxy seems to be relatively undisturbed, with no obvious signs of a major merger event or significant tidal interactions.
