The galaxy presents a generally smooth and elliptical morphology. Its light distribution is concentrated, with a noticeable central bulge. The color index suggests a population of older stars, as indicated by the reddish-yellow hue. There are no distinct spiral arms or prominent dust lanes visible, implying a relatively quiescent state of star formation. Faint disturbances may exist, suggesting a possible past or ongoing minor interaction or merger event. The galaxy shows a generally round appearance, with a hint of elongation.