The galaxy presents as a central, concentrated luminosity, surrounded by a more diffuse and extended halo. The core appears relatively smooth, showing a concentration of older stellar populations, indicated by the redder hue. The outer regions of the galaxy exhibit some irregularities and extensions, potentially indicative of tidal interactions or ongoing accretion events. There may be evidence of minor disturbances in the overall morphology, perhaps due to a previous or ongoing minor merger event. There is an indication of a small companion galaxy close to the main body which appears red. The color gradient suggests moderate levels of ongoing star formation, primarily occurring in the outer regions of the disk, though the global star formation rate is relatively low. The overall shape of the galaxy is intermediate between round and elongated, displaying a somewhat flattened structure.
