The galaxy presents as a highly inclined, late-type spiral, nearly edge-on, with a prominent central bulge. The bulge appears smooth and concentrated, exhibiting a yellowish hue suggestive of an older stellar population. A faint, extended disk is visible along the major axis, with hints of possible dust lanes or spiral arm structure, though resolution is limited. The overall color is slightly red, indicative of a population of older stars. The galaxy's shape suggests a system that has not recently undergone a major merger event.
