The galaxy presents a generally smooth, elliptical morphology. It appears as a concentrated spheroid of light, with a gradual decrease in luminosity from the core outwards. There is no discernible spiral arm structure or obvious dust lane features. The galaxy's color profile suggests a population dominated by older stars, emitting predominantly in the redder wavelengths with some presence in the green wavelengths, and a comparatively lower output in the blue wavelengths. There is some indication of minor disturbances in its form but it is hard to fully resolve. The object appears to be generally round, with a slight, almost cigar-like shape.
