The galaxy presents a somewhat elliptical morphology, suggesting a classification leaning towards the E type galaxies. The light profile appears relatively smooth, with no immediately obvious spiral arm structures or prominent dust lanes visible at this resolution. The central bulge region is clearly defined by a concentration of yellowish-white light, indicating the presence of an older stellar population. A faint, diffuse halo surrounds the central region, extending outwards and gradually fading into the background. The overall color suggests a moderate level of star formation, with the redder hues potentially indicating the presence of evolved stars and dust. No signs of significant tidal disturbances or ongoing major mergers are apparent.
