The galaxy exhibits a generally smooth morphology, with a slightly elongated, rounded appearance. It appears to be undergoing a possible minor merger, as indicated by the presence of a disturbed structure to one side of the main body, possibly a second nucleus or clump of stellar material. The galaxy's light profile is centrally concentrated, suggestive of an elliptical or lenticular type. The color gradient indicates that the central region has a yellowish tint, which may indicate an older stellar population, while the outer regions appear more blue-shifted. Overall, the galaxy appears to be a relatively massive system, likely with ongoing star formation activity indicated by the bluish hues. The galaxy shows signs of interaction, indicating a dynamic history possibly involving past or present tidal disturbances.
