The galaxy presents an overall diffuse appearance. A central, brighter region is evident, exhibiting a somewhat smooth texture. Surrounding this core, a fainter, more extended halo or disk-like structure is visible. The distribution of light suggests a spiral or possibly irregular morphology, although the resolution limits detailed classification. There is evidence of disturbed features, potentially indicating ongoing interactions or past mergers. Some bluer tinges are apparent throughout the galaxy and, in particular, some bluer colors exist more towards the outer arms.
