This galaxy presents as a somewhat elliptical or football shaped structure with a smooth overall appearance. The color gradient transitions from a more yellow/orange central region towards a bluer outer region. This suggests a potentially older stellar population concentrated in the core, with ongoing, but relatively low, star formation in the outer regions. There appears to be some asymmetry or minor disturbances in the galaxy's morphology, possibly indicating a past or ongoing minor interaction or merger event. The galaxy lacks a strong spiral arm structure or prominent dust lanes based on this observation.
