The galaxy appears as a centrally concentrated, relatively smooth object, exhibiting an elliptical morphology. A dominant yellowish-white hue suggests an older stellar population. There's a subtle, bluer tint visible in the outer regions, indicating the presence of some younger, hotter stars, possibly within a faint, disk-like component. The galaxy shows a relatively symmetrical distribution of light, with no obvious tidal features or signs of ongoing major mergers. Minor asymmetry is visible, potentially due to the presence of dust lanes obscuring parts of the galaxy. Overall, it has an intermediate redshift, with notable star formation.
