The galaxy presents as a smooth, elliptical or lenticular structure, with a noticeable central bulge. The luminosity profile appears concentrated towards the center, indicating a higher density of stars in the core region. There is a slight elongation to the galaxy's shape, appearing somewhat flattened. No distinct spiral arms or significant dust lanes are readily apparent. The color profile suggests a generally older stellar population with a yellowish or golden hue, consistent with relatively low ongoing star formation. There is no indication of any major tidal disturbances or mergers, suggesting a relatively undisturbed evolutionary history, or only minor disturbances. The galaxy appears well-defined, without any obvious signs of being an artifact or imaging error.
