The galaxy appears as a moderately bright, elongated object. Its morphology suggests a relatively smooth profile, though there is evidence of a subtle disk-like structure or possibly tidal disturbances. The central region shows a concentration of light, potentially indicative of a galactic bulge or a supermassive black hole actively accreting matter. The galaxy exhibits a color gradient, transitioning from bluer hues in certain areas to redder tones in others. This may be related to the distribution of stellar populations within the galaxy, with bluer regions potentially hosting younger, hotter stars and ongoing star formation. There is a possibility of ongoing or recent merger activity given the irregular shape. The color suggests that the galaxy is relatively massive and actively forming stars, although this activity might be moderate. The overall light distribution suggests that the galaxy is not perfectly symmetric and might be in the process of dynamically evolving.
