The galaxy presents as an oblong-shaped object with a centrally concentrated bulge. The bulge region appears yellowish-white in color, indicating a potentially older stellar population. The surrounding disk shows a bluer hue, suggesting the presence of younger stars and ongoing star formation. The disk exhibits some irregularities in its structure, but no major disturbances or interactions are visible. The overall morphology appears intermediate between a spiral and an elliptical galaxy, with a relatively smooth texture. The galaxy does not appear perfectly circular; it is elongated in shape. Evidence of potential minor disturbances is present in the disk, but no clear signs of any merging are apparent.
