The galaxy presents as a somewhat elliptical, moderately bright object. A central bulge is discernible, exhibiting a yellowish hue, suggesting an older stellar population. The surrounding disk appears relatively smooth, with a bluer color compared to the bulge, potentially indicating ongoing star formation. There are no obvious spiral arm structures visible. The overall morphology indicates a galaxy with a dominant spheroid component. The isophotes appear relatively regular, with no signs of major disturbances or ongoing mergers. The galaxy's axial ratio suggests it is viewed at a moderate inclination.
