The galaxy exhibits a flattened, somewhat irregular morphology. A prominent feature is a bright central region that is distinctly delineated from the rest of the galaxy. This central region shows a ringed structure, potentially indicative of past or ongoing interaction. The overall color distribution suggests the presence of both older stellar populations, contributing to the redder hues, and younger, bluer stars, particularly noticeable within the central region and a faint arm extending outwards. There appears to be some asymmetry in the distribution of the stellar populations. There is evidence of possible tidal features or distortions which may indicate a prior minor merger event. The majority of the disk has a smooth appearance.
