The galaxy presents as a relatively compact object with a generally smooth morphology. It displays a slightly elongated shape, appearing neither perfectly spherical nor highly flattened. The central region exhibits a higher surface brightness than the outer regions, suggesting a concentration of stars toward the galactic nucleus.

The galaxy appears to be dominated by older stellar populations, as indicated by its yellowish-red hue. However, there is a faint blue halo surrounding the central bulge, which hints at the presence of some younger, hotter stars and possible recent or ongoing star formation.

There is no clear evidence of spiral arms or a well-defined disk structure. Nor is there any indication of a major ongoing merger event, though some minor asymmetry or disturbance may be present in the overall shape.
