The galaxy appears as an elliptical-like structure with a smooth, diffuse light distribution. There is a concentration of light towards the center, exhibiting a bright, compact core region. The outer regions show a gradual fading of light intensity. The galaxy's overall shape is elongated, appearing neither perfectly spherical nor highly flattened. There are no apparent signs of strong spiral arm structures or significant dust lanes. There is little evidence of ongoing major merging activity, although subtle asymmetries and minor disturbances may be present upon closer examination. The galaxy's color suggests a relatively older stellar population.
