The galaxy presents as a centrally concentrated object with a generally smooth morphology. It appears relatively round, exhibiting a slight elongation. The color profile is dominated by yellowish hues, suggesting an older stellar population. There's a subtle gradient in color from the center outwards, with the core appearing more intensely yellow and transitioning to redder shades in the outer regions. There is no strong evidence of spiral arms or significant dust lanes, indicating this galaxy is likely to be an elliptical galaxy. There are hints of minor disturbances. Based on its red hue, we can hypothesize that star formation is likely at a low rate. The overall appearance suggests a well-evolved system.
