The galaxy presents as a relatively smooth, elliptical morphology. It displays a bright, concentrated central bulge exhibiting a yellow-orange hue, potentially indicative of an older stellar population. Moving outward from the core, the light gradually diminishes, transitioning into a fainter, more diffuse halo. The overall shape appears to be somewhat elongated but generally tending towards round, rather than a highly flattened disk-like structure. There is no clear evidence of spiral arms or significant dust lanes. No signs of any major merging events or strong tidal disturbances are visible, although there may be some minor distortions in the outer regions. Star formation seems to be minimal.
