The galaxy appears as a diffuse, elongated object with a moderate degree of smoothness. It exhibits a central concentration of light, though the structure appears relatively homogenous without distinct spiral arms or a prominent bulge. The overall shape could be classified as somewhere between rounded and cigar-shaped. The color profile suggests a galaxy with a population of older stars, as the light is redder in the r and z bands compared to the g band. No major mergers or significant disturbances are readily apparent in the galaxy's morphology, though the presence of minor disturbances cannot be ruled out based on this imagery alone. There is a subtle color gradient across the galaxy's extent, with possibly slightly bluer regions in the outer areas, indicating some ongoing, albeit low, star formation. The estimated size is consistent with a smaller, less massive galaxy.
