The galaxy exhibits a generally smooth morphology, with some subtle features suggesting a possible disk or internal structure. It displays a roughly elliptical shape, leaning towards a round appearance rather than a highly elongated or cigar-like form. There is an indication of moderate disturbance within the galaxy, but no obvious signs of a major ongoing merger event. The galaxy appears to be of significant size and mass and is actively forming stars. The colors suggest a mix of stellar populations, with some regions possibly hosting younger, bluer stars indicating recent or ongoing star formation, while other regions appear redder and may be dominated by older stellar populations. The presence of features suggests the possibility of past interactions or internal processes that have shaped its current appearance.
