The galaxy presents as a somewhat elongated, elliptical-like structure. Its central region exhibits a concentrated, bright core, with the intensity gradually diminishing toward the outer edges. The light distribution appears smooth, suggesting a relatively evolved stellar population. The color profile shifts from a yellow-orange hue in the core to a more muted color in the outer regions. The overall morphology lacks any distinct spiral arm structures or prominent dust lanes. There are also hints of a tidal tail.