The galaxy presents as a relatively compact object with a generally smooth appearance. Its overall shape is approximately elliptical, tending towards round, with a slight elongation. The central region is brighter and more concentrated than the outer regions. While the bulk of the galaxy appears largely featureless, there are subtle indications of possible disturbances or irregularities in the galaxy's morphology. A minor, asymmetric extension or plume-like feature is suggested. There are multiple clumps of increased brightness, potentially indicating ongoing star formation, with a moderate concentration towards the center. The galaxy displays a color gradient with the central bulge being a redder color than the edges. Based on the morphology there is evidence for a previous or ongoing merger.
