The galaxy presents as a somewhat elliptical structure. The central region exhibits a brighter, more concentrated luminosity, which decreases towards the outer edges. A slight disk structure may be present, but it is difficult to discern. The overall color profile suggests a mix of stellar populations. The central region appears more blue, hinting at possible star formation, while the outer regions are more red, possibly indicating a greater presence of older stars. Some faint irregular features are visible, suggesting the potential for minor tidal interactions or internal disturbances. The shape is primarily round, with minimal elongation. There is no strong evidence of a major merger or significant ongoing interactions, though subtle disturbances suggest mild gravitational activity.