The galaxy presents an elliptical morphology, though not perfectly spherical, appearing somewhat elongated with a cigar-shaped form. Its structure is largely smooth and lacks prominent spiral arms or distinct features, with an amorphous distribution of light. A small and concentrated central bulge of higher luminosity is visible. The light profile suggests a relatively evolved stellar population, exhibiting more light in the redder bands than the bluer bands. Faint indications of a disk-like structure may be present around the central region. There is a subtle indication of a possible minor disturbance to the galaxy's overall form. Its estimated size is moderate.