The galaxy presents as an elliptical morphology when viewed from our perspective, exhibiting a notable disk-like structure with an apparent axial ratio of approximately 0.36. The major axis of the galaxy is oriented roughly northwest to southeast.

The central bulge region shows a concentration of older stellar populations, indicated by the yellow-orange color. Moving outward from the core, a distinct disk component is visible, displaying a bluer hue suggesting the presence of younger, hotter stars and ongoing star formation regions. However, dust lanes are not readily apparent in this image. The color gradient implies a possible inside-out quenching of star formation within the disk.

The galaxy appears relatively undisturbed, showing no clear signs of tidal tails or distortions typically associated with recent major mergers, though the slight disturbance fraction may indicate some minor interactions in the past.
