The galaxy presents as a luminous, centrally concentrated spheroid. It exhibits a generally smooth morphology, with minimal evidence of spiral arm structure or prominent dust lanes. The light profile appears to be relatively symmetric. The core is bright and yellow, which may be due to aging stars. It may be on the larger side, at approximately 4.5 kpc radius. There is no obvious sign of ongoing merging activity. The galaxy exhibits a moderate redshift value, suggesting a significant distance from the observer.
