The galaxy presents as a largely featureless, smooth light distribution. It appears to be elliptical in shape, exhibiting a round to slightly elongated morphology. The central region is brighter and more concentrated in luminosity than the outer edges, indicating a possible bulge component. There is no obvious dust lane, spiral arm, or other notable feature visible in the image. The color profile suggests a relatively homogenous stellar population. The galaxy is most likely a quiescent system with a moderate stellar mass and rate of star formation.
