The galaxy presents a generally smooth morphology with a dominant central bulge. The overall shape is elliptical, tending toward a moderately rounded appearance, but not perfectly spherical. There is a slight elongation or cigar shape to the galaxy. Faint disk-like features extend away from the bulge, but the overall structure lacks prominent spiral arms.

There are no obvious signs of a major merger in progress; however, there appears to be minor asymmetrical disturbance in its outer regions, possibly related to tidal interactions or a minor merger event. This could be indicative of recent or ongoing accretion. The color gradients suggest a population of older stars, with little to no recent star formation visible in the main body. Some blue emissions exist within the disk.
