The galaxy presents as an elliptical system, moderately elongated in shape, with an approximate axis ratio of 0.6. Its overall color profile indicates a population of older stars, with a central region exhibiting a yellowish-white hue, suggesting a concentration of evolved stellar populations. The outer regions of the galaxy appear redder, potentially indicating the presence of dust lanes or a population of older, cooler stars. There is little evidence of spiral arm structure, nor are there any obvious signs of active star formation regions. The galaxy appears relatively smooth in texture, without significant irregularities or tidal features indicative of recent major mergers. The light is concentrated towards the center, gradually decreasing towards the edges of the system.
