The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution transitions gradually from the core outwards, suggesting a lack of distinct spiral arm features. The core region is bright and appears yellowish-white, potentially indicating an older stellar population. The overall shape is somewhat elongated rather than perfectly spherical. There is a slight asymmetry in the outer regions, perhaps hinting at a minor interaction or disturbance, but no major merger events are immediately obvious. The galaxy appears to be relatively isolated in its field.
