The galaxy presents a generally smooth morphology, with a predominantly elliptical shape that tends towards roundness. The light distribution appears largely homogeneous across the galaxy's body. There is faint suggestion of a bulge. There also appears to be a slight tidal disturbance. The galaxy exhibits a color gradient, with the central region appearing slightly redder than the outer regions, indicating potentially older stellar populations concentrated towards the core. No strong evidence of spiral arms or a distinct disk structure is discernible.
