The galaxy presents as a concentrated, elliptical form. The central bulge is prominent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Moving outward from the core, the color transitions slightly to a cooler, greenish tint, possibly indicating a small presence of younger, hotter stars or ionized gas in the outer regions. The overall structure appears relatively smooth, lacking the distinct spiral arms commonly observed in disk galaxies. The shape is elongated, and is most likely a disk galaxy viewed at an angle. There are some subtle asymmetries, hinting at possible past minor interactions or disturbances.
