The galaxy appears to be an elliptical type, characterized by a smooth, centrally concentrated light distribution. There is a lack of distinct spiral arms or a well-defined disk structure. The galaxy's overall shape is somewhat elongated, with an axis ratio less than one, suggesting a degree of flattening. Color gradients are subtle, with a slightly yellower hue toward the galactic center, indicating a possible higher concentration of older stellar populations in the core region. There are no obvious signs of active star formation or prominent dust lanes. The overall morphology suggests a relatively evolved system that may have undergone significant merging activity in its past.