The galaxy presents as a fairly compact and smooth object. The galaxy has a largely elliptical shape, appearing highly rounded. There is a concentration of light towards the center, with a gradual decrease in intensity outwards. The galaxy's color profile indicates a redder hue, which may suggest an older stellar population or the presence of dust obscuring bluer light from younger stars. There is no strong evidence of spiral arms or a distinct disk component. Signs of any ongoing or recent merger events are not obvious from this image. It appears to be an isolated system without significant interactions. Overall, the observed features suggest a more evolved galaxy, potentially a lenticular or elliptical type, with a dominant bulge.
