The galaxy presents as a moderately luminous elliptical or lenticular system at a redshift of approximately 0.157. It exhibits a generally smooth, centrally concentrated light profile with a slight elongation, suggesting a degree of flattening but without a pronounced disk component. The primary color is a yellow-orange hue, likely indicating a dominant population of older stars with limited on-going star formation. A subtle hint of bluer light is present in the central region, possibly indicating a small population of younger stars or an active galactic nucleus. There is no evidence of strong spiral arm structure, bar features, or significant tidal disturbances, suggesting this is a relatively isolated galaxy that has not recently undergone a major merger event. There is no substantial dust lane present.
