The galaxy presents a somewhat elongated, elliptical morphology. The central region exhibits a concentrated, bright core with a yellowish hue. The color suggests an older stellar population. A smoother, less defined halo surrounds the core, fading outwards. There is a very slight asymmetry or minor perturbation observed in the structure, suggesting a possible past interaction or disturbance. There is weak color variation indicating some presence of blue stars which suggests ongoing star formation. Overall the galaxy has a well defined shape and does not appear to be undergoing any major merging events.
