The galaxy presents a generally smooth and rounded morphology. The light distribution is concentrated towards the center, suggesting a significant central bulge. There appears to be a slight asymmetry and diffuse extension, indicating a potential interaction or minor disturbance event. The color profile suggests a mix of stellar populations. The central region exhibits a yellowish hue which implies older stellar populations. Further from the core, it has regions that trend toward a redder hue. While the majority of the light is smoothly distributed, there are faint indicators of possible tidal features, hinting at past or ongoing interactions.
