The galaxy presents as an object with a relatively smooth light distribution. The central region exhibits a bright, concentrated core that gradually diminishes in intensity towards the outer edges. There appears to be some asymmetry in its morphology, possibly indicating the presence of a faint, distorted spiral arm structure or tidal features resulting from a minor gravitational interaction. The color profile suggests a generally evolved stellar population, indicated by its redder hues, though there is evidence of bluer regions interspersed, potentially indicative of ongoing star formation. Overall, it seems to be a galaxy undergoing, or having undergone, morphological transformation.
