The galaxy presents a generally smooth, elliptical morphology. A central, moderately bright bulge is observed, exhibiting a slight elongation. The luminosity appears to decrease gradually from the bulge outwards, with no distinct spiral arms or prominent features readily apparent. The light distribution suggests that this galaxy may be either an elliptical galaxy of type E3-E5, or potentially a lenticular galaxy with a weak disk. Minor disturbances are not clearly apparent, but cannot be completely ruled out at this resolution. The overall shape is primarily round. The galaxy's color indices suggest the presence of a primarily older stellar population with a moderate degree of star formation activity.