The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be somewhat rounded in shape, though possibly slightly elongated along one axis. The central region exhibits a high concentration of light, suggesting a prominent bulge component. The color profile transitions from a yellowish hue in the core to a bluer tinge in the outer regions. This may imply a difference in stellar populations, with older, redder stars dominating the bulge and younger, bluer stars populating the outer regions. The overall texture of the galaxy is quite uniform with no clear evidence of spiral arms or significant dust lanes. There is no sign of ongoing major merging activity, although a very minor disturbance cannot be entirely ruled out.
