The galaxy appears as a relatively smooth, centrally concentrated elliptical or lenticular type. It exhibits a bright, yellowish core, suggesting an older stellar population dominating the central region. The light gradually decreases in intensity from the core outward, with a fairly symmetrical, circular or slightly elliptical morphology. There is a subtle hint of a surrounding disk-like structure, but no well-defined spiral arms or prominent dust lanes are visible. There is a slight suggestion of some blueish light within the outer regions, which suggests a small amount of ongoing star formation. Overall, the galaxy presents a well-ordered structure with no signs of significant tidal disturbances or ongoing major mergers.
