The galaxy presents a generally smooth morphology, with a somewhat elliptical shape. The light profile appears centrally concentrated, exhibiting a bright, yellowish core that likely hosts an older stellar population. Moving outward from the core, the light gradually fades, exhibiting a diffuse, bluer halo surrounding the central region. This halo may indicate the presence of younger stars. There's a hint of a possible faint disk structure, but it is not clearly defined, potentially indicating a galaxy transitioning from a spiral to an elliptical type, or a disk galaxy seen at an oblique angle. Evidence of any ongoing major mergers is not readily apparent, though subtle distortions or minor disturbances cannot be entirely ruled out. Overall, the galaxy appears relatively evolved, with a moderate mass, and low level of star formation.
