The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The color profile suggests a population of older stars, emitting primarily in the redder wavelengths. There's a slight color gradient observed, with the core appearing more yellow compared to the outer regions which exhibit a redder hue. The galaxy's morphology does not show any prominent spiral arms or disk-like features. There is a faint and diffuse halo surrounding the main body of the galaxy. No signs of active star formation or significant dust lanes are apparent from this imaging.
