The galaxy presents an elliptical morphology, appearing elongated in shape. Its surface brightness distribution is relatively smooth, with a gradual decrease in intensity from the central region outwards, suggesting a higher concentration of stars and gas in the core. The galaxy exhibits a blueish hue, particularly in the central region, indicative of ongoing star formation. There is no clear evidence of spiral arms or a well-defined disk structure. The galaxy appears to be a relatively isolated system, with no visible signs of tidal interactions or major mergers.
