The galaxy presents as an elliptical or lenticular type with a central bulge. The core exhibits a concentrated, bright luminosity indicating a relatively dense stellar population. The galaxy exhibits a somewhat amorphous shape. There is some subtle indication of a disk structure but no evidence of tightly wound spiral arms. The overall color of the galaxy appears generally redder, suggestive of an older stellar population, though there are some indications of blueish star formation regions within the galactic disk. There are faint asymmetries or disturbances, potentially caused by a minor gravitational interaction or merger with another smaller object, that are occurring, but they are not so prominent that there is a major disturbance. Overall, the image suggests a galaxy with both smooth and featured elements and an intermediate mass.
