The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. Its overall shape approximates a slightly flattened spheroid rather than a defined disk. The central region is brighter compared to the outer edges, hinting at a higher stellar density towards the core. There is no clear evidence of spiral arm structures or prominent dust lanes. There are hints of minor disturbances, likely a very recent merger, and the galaxy overall is relatively blue in color, and thus likely in a state of high star formation.
