The galaxy appears as a centrally concentrated object with a generally smooth morphology. It presents a bright, yellowish core that gradually diffuses into the surrounding galactic structure. There is little evidence of distinct spiral arms or prominent dust lanes, suggesting a relatively featureless disk or potentially an elliptical morphology. The galaxy exhibits a slightly elongated shape, deviating marginally from perfect circularity. Faint, extended regions surround the core, indicating the presence of a galactic halo or diffuse stellar population. No obvious signs of major mergers or tidal disturbances are visible in this image, though some minor asymmetry cannot be ruled out. The light profile suggests a fairly evolved system with a relatively low star formation rate. The color distribution indicates a mature stellar population, with the yellow hue suggesting older stars dominate.
