The galaxy presents as a generally smooth object, with a concentrated central bulge that appears approximately spherical. The light distribution is dominated by the yellowish color of older stars. There is some hint of a faint, diffuse disk surrounding the bulge. The presence of possible distortion or faint feature suggests a minor gravitational interaction. The galaxy appears relatively isolated. Overall, the morphology suggests a late-type disk or perhaps a transition between a late-type disk and an elliptical galaxy, leaning towards a more passive, less actively star-forming system.
