The galaxy appears as a single, relatively smooth object with a noticeable central concentration. The light distribution suggests an elliptical or lenticular morphology, with minimal discernible spiral arm structure. The color gradient transitions from a yellowish-white core to a bluer outer region, potentially indicating a mix of older stellar populations in the center and more recent star formation activity further out, though the blue color could also just be a result of dust absorption. The galaxy's overall appearance is moderately disturbed, possibly due to a recent or ongoing minor interaction. The galaxy has a generally round profile, with a hint of elongation but no extreme asymmetry.
