The galaxy presents as a somewhat elliptical structure, with a bright, concentrated central bulge. The light distribution suggests a higher concentration of older stars within the core, indicated by the yellowish hue. Moving outward from the center, the galaxy exhibits a gradual decrease in luminosity. There is some evidence of a faint, diffuse disk or halo extending beyond the central region, but it lacks prominent spiral arm features. The overall color is dominated by redder wavelengths, suggesting a relatively low rate of ongoing star formation. There are some indications of minor disturbances in the outer regions of the galaxy.
