The object presents as a galaxy with an overall elongated morphology, appearing as a flattened spheroid. There is a bright, concentrated central bulge which dominates the overall luminosity profile. Moving outwards from the center, a disk-like component can be observed. This disk appears to be tilted at an oblique angle relative to our line of sight, presenting a partially edge-on perspective.

There is no clear indication of well-defined spiral arms or a bar structure within the disk. The disk component exhibits a mottled texture, potentially indicative of patchy star formation regions or dust obscuration. The overall color of the galaxy appears relatively consistent, with a slight blueish hue, possibly indicating the presence of younger stars in its features. Irregular features are apparent, which point towards a potential ongoing or recent minor merger event. No obvious tidal tails or extensive debris fields are immediately discernible in this field of view.