This galaxy presents a roughly elliptical morphology, exhibiting a smooth, diffuse appearance rather than distinct spiral arms or a well-defined disk structure. The central region displays a pronounced concentration of light, suggesting a significant stellar population and potentially a supermassive black hole actively accreting material.

The color gradient transitions from a yellowish-orange core, indicative of older, cooler stars, to a bluer halo, possibly containing younger stellar populations and ongoing star formation. Although the image resolution limits detailed analysis, there is subtle irregularity in the outer regions that could be signs of gravitational interactions or minor disturbances. The galaxy appears relatively isolated, without any clear evidence of ongoing major mergers, though faint tidal features cannot be ruled out. It is a relatively luminous galaxy, with a mass that is on the larger end. It is currently undergoing moderate levels of star formation.
