The galaxy presents a predominantly smooth morphology. It exhibits a roughly circular shape, appearing mostly rounded with a slight deviation towards an intermediate form. The galaxy's light is concentrated towards the center, suggesting the presence of a significant bulge component. Faint color variations exist within the galaxy, with the central region appearing slightly more yellowish. This coloration may indicate an older stellar population. No prominent spiral arms or other distinct features are visible. There is no strong evidence of any significant ongoing merging activity or major disturbances, with only a very slight possibility of minor disturbance. Overall, the galaxy appears to be a relatively quiescent system.
