The galaxy presents as a centrally concentrated, elliptical-like structure. The core is a bright, yellowish-white, suggesting an older stellar population. This central region gradually fades into a less intense reddish hue toward the outer edges. The galaxy appears relatively smooth, with no discernible spiral arms or obvious dust lanes. It seems fairly undisturbed, showing no major signs of a recent merger or significant tidal interactions. Faint extensions or distortions are not readily apparent in the surrounding space. The galaxy exhibits a moderate redshift, indicating a substantial distance. The size of the galaxy appears moderate, but with some uncertainty due to the limited resolution. Overall, it is suggestive of a fairly evolved elliptical or lenticular galaxy with a dominant older stellar population and low levels of ongoing star formation.
