The galaxy presents a largely smooth morphology with little discernible structure. Its shape is noticeably elliptical, deviating somewhat from a perfectly circular form. The core region appears bright and concentrated. A smooth, diffuse halo surrounds the central core, diminishing in intensity with increasing distance. The overall color profile suggests a population of older stars, with a subtle bluish tint that might indicate a small degree of recent star formation activity. There is no clear evidence of spiral arms or prominent dust lanes. The galaxy shows no signs of ongoing major merging events, though subtle disturbances cannot be entirely ruled out.
