The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a concentrated, brighter, yellowish-white hue, indicative of an older stellar population. The outer regions appear less luminous, fading into a blue color, indicating a more sparse distribution of stars and potentially younger stellar populations. The overall shape is elongated, approximating a cigar shape, suggesting an elliptical galaxy type seen from an angle. There is no visible evidence of spiral arms or significant dust lanes. No clear signs of ongoing major mergers or tidal disturbances are apparent, though a minor irregularity on the outskirts is not out of the question.
