The galaxy presents a primarily smooth morphology. The central bulge appears dominant, exhibiting a concentrated, bright yellowish-white color, indicative of an older stellar population. Moving outward from the core, the galaxy exhibits a subtle disk-like structure, though less pronounced, with a slightly fainter and redder hue. There is a hint of internal structure within the galaxy, with some faint irregularities suggesting possible minor disturbances or mergers in its past. The overall shape is somewhat elliptical, deviating from a perfect circular form, but it is not excessively elongated. The color suggests a relatively moderate level of ongoing star formation.
