The galaxy appears to be a relatively smooth, elliptical-like object with a concentrated central bulge. The galaxy exhibits a noticeable color gradient, transitioning from a yellowish-white core to a slightly redder outer region. This may indicate a centrally concentrated population of older stars and dust, with a decreasing age gradient towards the outer edges. There is a hint of a potential tidal disturbance or asymmetry, suggested by a slightly elongated or distorted shape. The system does not appear to be undergoing a major merger. Some level of star formation is likely occurring, but at a low rate. The galaxy exhibits a high degree of central concentration.
