The galaxy presents a relatively smooth, elliptical morphology. It exhibits a central bulge region that appears more concentrated and brighter, fading outwards towards the edges. The overall shape is elongated, tending towards a cigar-like appearance. There are some hints of disturbances in the outer regions, potentially indicating ongoing or past minor interaction events. The galaxy is largely featureless, lacking prominent spiral arms or distinct dust lanes. Color gradients suggest an older stellar population, with a general reddish-orange hue dominant across the galaxy. The outer regions appear slightly bluer, possibly indicative of some younger stars but these are subtle. There is no definitive evidence of active star formation, although its presence cannot be completely ruled out based on the color composition. No significant signs of a major merger are obvious.
