The galaxy presents a generally smooth and rounded appearance. The core exhibits a bright, concentrated central region that fades outwards into a more diffuse halo. There is little evidence of spiral arm structure or significant dust lanes, though subtle color variations may indicate the presence of some subtle disk-like features. The color profile suggests an older stellar population, particularly in the core, with a redder hue overall. A slight flattening is observed, indicating it is not perfectly spherical. There's a subtle suggestion of a slight disturbance in the overall light distribution, but no clear signs of ongoing major merging activity.
