The galaxy presents as a smooth, elliptical structure with a concentrated central bulge. There is a noticeable elongation in its overall shape, tending towards a cigar-like appearance. The color profile indicates a predominantly older stellar population, with a yellow-red hue dominating the central region, possibly indicative of minimal current star formation in that area. Fainter, bluer tendrils can be seen extending from the central area and towards the edge of the galaxy, which suggests a small amount of on-going star formation. There are no obvious signs of a major ongoing merger. There may be some minor disturbance in the morphology of the galaxy. Overall, the galaxy appears to be an evolved system transitioning to a more quiescent state.
