The galaxy presents a roughly elliptical morphology. It appears relatively smooth in structure, with a bright, concentrated central bulge that dominates the overall light emission. The surrounding disk shows a slight flattening. There is some suggestion of faint, diffuse spiral arms extending outwards from the central bulge, but they are not well-defined. The colour gradient suggests a possible presence of younger stellar populations closer to the core, with a colour shift towards redder hues in the outer regions. There may be faint disturbances in the disk, possibly indicating a minor interaction with another galaxy or some degree of internal instability, but this needs further investigation to confirm.
