The galaxy exhibits an elliptical morphology, appearing elongated rather than perfectly spherical. Its light distribution is concentrated towards the center, which is noticeably brighter than the outer regions. The core appears smooth and lacks any discernible distinct features such as spiral arms or bars. The overall color profile suggests a population of older stars, with a generally redder hue dominating the galaxy's light. Faint, diffuse extensions are visible surrounding the main body of the galaxy, suggesting a possible halo or tidal features, although no major distortions or signs of recent mergers are immediately apparent. There is a slight color gradient, with bluer colors around the edges of the galaxy suggesting the presence of some younger stars or ongoing star formation. Overall, this galaxy presents as a relatively quiescent, early-type system.
