The galaxy presents as a flattened, elliptical morphology. It is oriented with its major axis nearly horizontal in the image. There is a notable central bulge appearing more concentrated and luminous than the outer regions, with an orange hue. Several distinct, brighter knots or clumps are scattered throughout the galaxy's disk, some also having a similar orange color. These may indicate regions of active star formation or dense stellar populations. There is some minor visual disturbance, possibly indicative of an ongoing merger. A smooth quality is observed, however the irregularities lead me to believe it could be a merger. The overall color is a mix of yellow and orange, implying a population of older stars or significant dust obscuration, though regions of bluer emission are not entirely absent.
