The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing bright yellow, suggesting a population of older stars. Moving outward from the core, the light gradually diminishes, transitioning to a redder hue, potentially indicating a lower density of stars or a different stellar population. There's a hint of a flattened disk, but the galaxy lacks distinct spiral arms or prominent features typically associated with spiral galaxies. The overall form appears largely undisturbed, with no readily apparent signs of recent major mergers or tidal interactions. The galaxy has a generally round shape, with hints of a cigar shape.