The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The overall shape appears largely elliptical or lenticular, showing a high degree of radial symmetry. A faint disk may be present, though it is not clearly defined, and no spiral arms are visible. The color gradient suggests a population of older stars, as the central region exhibits a yellow hue. There is no obvious evidence of ongoing major star formation or significant dust lanes. The galaxy shows little visual signs of interaction or recent merger events, appearing relatively undisturbed. Its structure is compact, with a definite concentration of light toward the center, indicating a high stellar density.
