The galaxy appears as a moderately luminous, elongated object. It exhibits a smooth, diffuse morphology with a noticeable central bulge that gradually fades into the outer regions. The overall shape can be described as cigar-shaped. There's no immediately discernible evidence of spiral arm structure or significant dust lanes within the galaxy. The color profile suggests an older stellar population, displaying a yellowish hue in the central regions, transitioning to slightly bluer tones towards the edges, possibly indicating some ongoing, albeit subdued, star formation in the periphery. There are no signs of active galactic nuclei activity or interactions with other galaxies in its immediate vicinity. Overall, the galaxy seems to be an elliptical, or possibly lenticular, system with a fairly high degree of central concentration.
