The galaxy appears to be a moderately luminous elliptical galaxy at a redshift of approximately 0.28. Its overall morphology is smooth, with no distinct spiral arms or bar structure apparent. The color profile suggests an aging stellar population, with a redder hue indicative of older, less massive stars dominating the light output. There is a slight elongation in its shape, appearing somewhere in between round and cigar shaped. No signs of major ongoing mergers are observed, though subtle disturbances cannot be ruled out. There is no dust lane visible. The galaxy presents a centrally concentrated luminosity profile, decreasing smoothly outwards. Star formation activity is low.
