The galaxy appears as a concentrated, roughly elliptical structure. It presents a smooth overall appearance, with a high degree of central concentration. There is a general lack of distinct spiral arm features or prominent dust lanes. The color profile is somewhat consistent, though with a slight gradient indicating a higher concentration of older stellar populations at the core, exhibiting a yellow/orange hue. There's no strong evidence of ongoing major merger activity, though subtle irregularities in the outer regions may point towards minor disturbances or past interactions. The galaxy exhibits a moderate degree of roundness, appearing neither perfectly spherical nor significantly elongated.
