The galaxy presents as an elongated, disk-like structure, viewed at a significant inclination. There is evidence of a central bulge, though it is not particularly prominent. The disk exhibits a generally smooth texture without clear indications of spiral arm structures, suggesting a more evolved morphology. The color gradient across the galaxy shows a transition from bluer tones in the outer regions of the disk towards a slightly redder hue in the central bulge, possibly indicating older stellar populations concentrated towards the center. The overall appearance suggests the possibility of an elliptical galaxy, or a spiral galaxy with tightly wound arms. There appear to be slight asymmetries or disturbances in the outer edges of the galaxy, potentially indicating minor gravitational interactions. The light is generally faint, indicating this is a galaxy with a modest amount of star formation activity or is a smaller galaxy.
