The galaxy exhibits a generally smooth morphology, appearing largely featureless upon visual inspection. Its shape approximates a circular form, showing high degree of roundness, but the light may have artifacts in the data. A central bulge is discernible, characterized by a concentrated region of light. The overall color profile suggests a relatively older stellar population, but there is evidence of a localized bluer region near the center, which could suggest recent star formation in the nuclear area. No prominent spiral arms or bar structures are immediately obvious, and no signs of major galactic mergers. Marginal disturbances or minor disturbances could be present.
