The galaxy presents as a relatively compact object. Its overall shape appears slightly irregular, possibly indicating a past or ongoing interaction. There's evidence of both a smooth, concentrated central region and fainter, more diffuse features extending outwards. The central region exhibits a yellowish-white hue, suggesting a population of older stars. Surrounding the central region, there's a bluer component. The bluer regions may indicate younger stellar populations and ongoing star formation. The distribution of light is not uniform, with some areas appearing brighter and more concentrated than others. The outer regions show faint hints of disturbed structure.
