The galaxy presents as a luminous, centrally concentrated object with a roughly elliptical morphology. It exhibits a smooth, featureless appearance, lacking any distinct spiral arm structures or prominent dust lanes. The light distribution suggests a relatively well-mixed stellar population, and a dominance of older stars. Color gradients appear subtle, with a somewhat redder hue in the central regions transitioning to slightly bluer tones in the outer halo, suggestive of ongoing or recent low levels of star formation at larger radii. The shape is neither perfectly round nor elongated, showing some characteristics of both round and cigar shaped galaxies. There is no indication of any major merger events, though the image resolution does not preclude the possibility of minor disturbances.
