The galaxy presents as a somewhat diffuse, lenticular-like structure with a centrally concentrated bulge region surrounded by a flattened disk. The overall morphology appears relatively smooth, with a slight elongation suggesting an elliptical or possibly edge-on spiral nature. Evidence of a spiral structure is not immediately apparent, with no obvious arm structures visible. The color profile shows a central bright, slightly blueish hue, possibly indicating ongoing star formation. The outer disk exhibits a more redish hue suggesting an older stellar population and/or dust obscuration. There may be a minor disturbance, such as a slight asymmetry in the disk, but evidence is inconclusive. There is no evidence for a major merging event. Overall, the galaxy appears to be a relatively evolved system with an intermediate mass.
