The galaxy presents a generally smooth morphology, appearing as an elliptical or lenticular type. It displays a moderate axis ratio, appearing somewhat elongated but not highly flattened. The galaxy's light profile suggests a centrally concentrated spheroid with a gradual decline in surface brightness towards its outer regions. There may be very minor disturbances, but overall, the galaxy exhibits a well-defined structure, without prominent spiral arms or irregular features. Color gradients are visible, with the central region appearing slightly redder than the outer regions, suggestive of an older stellar population at the core. The galaxy is of intermediate luminosity, as determined from the apparent magnitude and redshift, and exhibits low-to-moderate star formation activity.
