This galaxy appears as a relatively smooth, elliptical-shaped object. It is likely a mature galaxy, showing a lack of prominent spiral arms or active star-forming regions. The color profile suggests a predominantly older stellar population, with a yellowish-orange hue dominating the core and gradually fading towards the outer regions. There may be minor disturbances in the galaxy's morphology, perhaps due to a past merger event or ongoing gravitational interactions. However, these do not appear to be dramatically disrupting the galaxy's overall structure. The galaxy seems fairly isolated, with no close companions clearly visible in the immediate vicinity, though higher resolution imaging might reveal fainter tidal features or satellite galaxies.
