The galaxy presents as a generally smooth, elongated structure. It exhibits a prominent central bulge region with a concentrated, bright core. The light emanating from the galaxy is not uniform, displaying a noticeable color gradient. The core appears yellower, possibly indicating an older stellar population, whereas the outer regions show a bluer hue suggesting the presence of younger, hotter stars and ongoing star formation. The overall morphology suggests an elliptical or lenticular classification. There is no apparent spiral arm structure or dust lane obscuration evident in this image. A slight asymmetry in the outer halo could indicate past or ongoing interactions with a smaller satellite galaxy but this would need to be confirmed by further more detailed imaging. The galaxy appears relatively isolated, exhibiting no significant signs of a major merger or tidal disruption.
