The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, diffuse morphology. The light distribution suggests a centrally concentrated spheroid, with a gradual decrease in luminosity outward from the core. There is little evidence of distinct spiral arms or prominent dust lanes. The overall color appears slightly reddish, suggesting a relatively older stellar population with lower ongoing star formation. There might be a slight asymmetry in the outer regions but it does not look like a major merging event. It is elongated, but largely appears as an individual object.
