The galaxy presents as a somewhat elliptical, diffuse object with a bright, concentrated central region. The core exhibits a yellowish-white hue, potentially indicative of an older stellar population dominating this region. Extending outwards from the core is a less concentrated, fainter halo of light. The color shifts slightly towards the blue end of the spectrum toward one end of the halo, suggesting the possibility of more recent star formation activity in that area. The morphology appears generally smooth, with no immediately obvious spiral arm structures or significant dust lane features. There may be some distortion or minor disturbance in the structure. The overall light distribution suggests a system that is relatively evolved.
