The galaxy presents as a relatively smooth, centrally concentrated light distribution. The core appears nearly spherical in shape, with a general lack of distinct spiral arm structures or prominent dust lanes. There are hints of asymmetry in the galaxy's overall form, potentially indicating some past interaction. The color profile suggests a galaxy dominated by older stellar populations, exhibiting a reddish-yellow hue throughout the majority of its body. A small region exhibits a bluer color profile, suggesting a small area of recent star formation. Overall, the galaxy appears to be in a relatively quiescent state with minimal ongoing star formation.
