The galaxy presents as a centrally concentrated, moderately luminous object. The morphology appears largely smooth, lacking prominent spiral arms or a well-defined disk structure. The light distribution indicates a roughly elliptical shape, tending toward a spheroid, although not perfectly circular. There is a slight elongation evident. The color profile suggests a population of older stars, exhibiting a redder hue overall, with a brighter, bluer core. Subtle irregularities in the outer regions hint at possible minor disturbances, although no major merger events are readily apparent. Star formation is occurring at a modest rate. The galaxy's mass is estimated to be substantial.
