The galaxy presents a slightly elliptical morphology, with the major axis oriented approximately northeast to southwest. The central region exhibits a concentrated, reddish hue, suggesting an older stellar population and/or significant dust obscuration. Surrounding this core is a more extended, diffuse disk-like structure. This disk shows a color gradient, shifting towards a greenish-yellow hue with increasing radius from the center, potentially indicating a mix of younger stars and ongoing star formation activity. The disk appears relatively smooth, without obvious spiral arm structures. The overall appearance is consistent with that of a lenticular or early-type spiral galaxy, though with a noticeable disk component. There is no clear evidence of strong tidal features or ongoing major merger activity, suggesting it is a relatively isolated and undisturbed system.
