The galaxy appears as a moderately luminous object with a smooth, elliptical morphology. It exhibits a concentrated central bulge and a generally featureless disk, lacking prominent spiral arms or dust lanes. The color profile suggests a dominant population of older stars, indicated by the redder hue, with a low star formation rate. The object displays a moderate elongation, appearing more lens-shaped than perfectly spherical. There is some indication of minor gravitational disturbance, with possible tidal features or asymmetries within the galaxy's outer regions, though these are not strongly pronounced. There is no evidence of an active galactic nucleus or other high-energy phenomena within the image.
