The galaxy exhibits a morphology suggestive of a recent or ongoing interaction, potentially a merger. A central, luminous component appears relatively smooth and elliptical, with a noticeable yellowish hue, indicating a population of older stars and a lack of significant ongoing star formation. Extending from this core is a fainter, more diffuse component. This secondary component is bluer in color, potentially indicating more recent star formation. There is a noticeable tidal tail or extended feature emanating from one side of the galaxy. The overall shape of the galaxy is elongated, and there appears to be an interaction between the elliptical central component and the disk. There is no apparent dust lane.
