The galaxy presents a generally smooth appearance, lacking prominent spiral arms or a well-defined disk structure. The light distribution is centrally concentrated, suggesting a dominant bulge component. The galaxy's shape is moderately elliptical, appearing as a somewhat elongated spheroid. The central region exhibits a yellowish-orange hue, possibly indicating an older stellar population. There are hints of bluer regions at the outer edges, potentially signifying areas of ongoing, albeit subdued, star formation. Overall, the galaxy gives the impression of an early-type system in a relatively quiescent state. Some slight distortions are visible, suggesting a past or ongoing gravitational interaction.
