The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. There is no discernible spiral arm structure or strong bar feature apparent within the resolution of this image. The galaxy is elliptical in form. A core region of moderate luminosity is visible, transitioning outwards to a less intense halo. The galaxy displays a slight colour gradient, shifting from a redder central hue to a bluer surrounding region, suggestive of differences in stellar populations. Given the smoothness and color profile, a significant portion of the stellar population is likely composed of older stars, particularly within the core. There are no readily apparent signs of ongoing major merger activity, though a minor disturbance or interaction cannot be entirely ruled out.
