The galaxy presents as a moderately luminous object with a concentrated central bulge and a flattened, disk-like structure. The light distribution suggests it is neither perfectly elliptical nor spiral, but rather an intermediate morphology. The central region exhibits a yellow-white hue, possibly indicating an older stellar population. There is a hint of bluer light in the outer regions of the disk, suggestive of ongoing or recent star formation, albeit at a relatively low rate. Some irregularities are visible within the galaxy's structure, possibly indicating minor gravitational interactions or disturbances. There is no definitive evidence of strong tidal tails or a major merger event, but a lopsidedness in the disk suggests a possible past interaction. The overall appearance points towards a galaxy that is not actively undergoing a major transformative event, but rather evolving relatively quiescently.
