The galaxy presents as a slightly elongated, elliptical-like structure. It exhibits a smooth, largely featureless appearance, lacking distinct spiral arms or a prominent central bulge. The color distribution suggests a generally older stellar population, with a concentration of redder hues towards the center, fading to slightly bluer tones at the periphery. There is little evidence of active star formation regions based on the image, suggesting a relatively quiescent state. The galaxy appears to be isolated, showing no obvious signs of ongoing merger activity or significant tidal disturbances in its immediate vicinity.
