The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge that fades outward into a more diffuse halo. The light profile suggests a relatively old stellar population, with a dominant yellowish-orange hue, indicating a lack of significant ongoing star formation. There is a suggestion of possible minor disturbances or faint tidal features that could indicate gravitational interaction with another galaxy at some point in its history. These features appear as subtle color asymmetries and deviations from a perfectly smooth light distribution. There are some faint, irregular regions or clumps around the galaxy, potentially dwarf galaxies being accreted or star-forming regions within the extended halo.
