The galaxy presents as a moderately bright, elliptical-shaped object. Its color gradient transitions from a yellowish-white central region to a dimmer, bluish-white periphery. The central concentration of light suggests a dense core, likely composed of older stellar populations. The smooth, featureless morphology indicates a lack of prominent spiral arms or dust lanes. The galaxy appears to be relatively isolated with no apparent signs of tidal disturbances or ongoing merger activity. Its overall form points toward a dynamically relaxed system, potentially an elliptical galaxy viewed at an oblique angle. The slight elongation hints at a possible cigar shape. The apparent size indicates that it is not particularly large, but its moderate luminosity suggests it is a galaxy of substantial mass. Given the color profile, the galaxy is likely undergoing minimal star formation.
