The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. The overall form appears generally round, with no obvious spiral arms or bar-like features visible. The light distribution decreases steadily from the core outwards, with no distinct breaks or features. There are no obvious signs of tidal tails or morphological disturbances indicative of a recent merger event, though the resolution is limited. Faint extensions are visible beyond the brighter central region, contributing to a relatively large overall apparent size. There are no easily discernible dust lanes or prominent star-forming regions within the visible extent of the galaxy. The color gradient suggests a lack of significant ongoing star formation across the disk, reinforcing the notion of a more evolved galaxy.
