The galaxy presents as a somewhat elliptical object with a bright, concentrated central bulge. There is a noticeable color gradient from the core to the outer regions. The central bulge exhibits a yellow-white hue, suggesting a population of older stars. The outer disk region appears slightly bluer, possibly indicating the presence of younger, hotter stars and regions of on-going star formation. The galaxy's overall light distribution is relatively smooth and diffuse, which suggests that it may be an early-type spiral galaxy. There is some evidence of a minor disturbance in the galaxy’s shape, possibly the result of a minor merger event or interaction with a smaller galaxy. Overall, the galaxy appears to be of moderate size.
