This galaxy appears to be a relatively smooth, elliptical system, exhibiting a concentrated central bulge. The light distribution indicates a dominant spheroidal component, with a near-circular isophotal shape. There is evidence of some variation in color across the galaxy, with a yellowish hue in the central region, transitioning to a slightly bluer color in the outer regions of the galaxy, though some redness is present. The system displays no obvious spiral arm structures or significant dust lanes. There is no indication of a ongoing major merger, though there may be some minor disturbances based on the slight color variation in the outskirts. The galaxy shows characteristics consistent with a post-starburst or quiescent system, though there is likely some ongoing star formation in the galaxy.
