The galaxy presents as an elliptical morphology, with a generally smooth light distribution and no readily apparent spiral arm structures or distinct dust lanes. The central region appears more concentrated and exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the light fades gradually, with the outer regions showing a slightly redder tint. The overall shape is somewhat elongated, but not highly flattened; it tends towards an "in between" shape and not an obviously cigar-shaped or round shape. There is no visual evidence of significant ongoing mergers or major disturbances in the galaxy's structure; the overall appearance is relaxed.
