The galaxy appears as a concentrated, centrally brightened object. Its overall morphology is largely smooth with a somewhat amorphous structure, lacking any prominent spiral arms or a well-defined disk. There is a slight ellipticity. The light distribution suggests a spheroidal component, potentially indicative of an elliptical galaxy or a bulge-dominated spiral. There's some subtle evidence of a faint, extended halo. There's no significant disturbance to the overall symmetry, suggesting it is likely not undergoing a major merger. The color appears relatively uniform across the galaxy, with a slight trend towards redder colors in the central regions. This could imply an older stellar population concentrated in the core. Based on the data there is some star formation present, but not at a high rate.
