The galaxy appears as a somewhat rounded structure, though not perfectly circular. Its light is distributed diffusely with a central concentration, suggesting a bulge. The primary color is reddish, with some regions appearing more blueish, possibly indicating areas of ongoing star formation. The galaxy does not present a well-defined disk, and no spiral arm structures are readily apparent. There's a noticeable absence of major disturbances or indications of merging activity, although subtle irregularities in its shape suggest the possibility of minor gravitational interactions in the past.
