The galaxy appears as a somewhat diffuse object with a bright central region. There are subtle irregularities within its structure, with evidence of a slight asymmetry or disturbance in the distribution of light. A faint, extended halo surrounds the central structure, exhibiting a gradient in luminosity that decreases with increasing radius. The colour profile indicates a bluer central region. There are possible indications of minor tidal interactions or recent mergers, though no dominant merger features are readily visible.
