The galaxy presents an elliptical morphology, exhibiting a smooth and largely featureless appearance. The central region displays a concentrated, yellowish-orange hue, indicative of an older stellar population. Moving outward from the core, the color transitions to a bluer tone, potentially suggesting the presence of younger stars and/or some degree of star formation activity, albeit not prominently. The overall shape is somewhat elongated but still relatively round. No significant signs of tidal disturbances, major mergers, or distinct spiral arms are visible. The galaxy appears relatively isolated.
