The galaxy presents an elliptical morphology, exhibiting a relatively smooth and concentrated light profile. The central region displays a bright, yellowish hue, potentially indicating a population of older, evolved stars. Moving outwards from the center, the light gradually diffuses, transitioning to a bluer color, suggesting the presence of a younger stellar population. No distinct spiral arms or bar structures are discernible within the galaxy's disk. The overall form approximates a circular shape, with only minor deviations from perfect symmetry. There appear to be signs of minor gravitational interactions, possibly slight irregularities. The colors suggest that this galaxy has medium levels of star formation.