The galaxy exhibits a relatively smooth morphology, lacking prominent spiral arms or a well-defined disk structure. Its light distribution is highly concentrated, suggesting an elliptical shape or a lenticular galaxy viewed close to face-on. The galaxy appears nearly round, with a slight hint of elongation. The color profile indicates a generally older stellar population, with a redder hue dominating the overall light. There is no discernible active galactic nucleus or intense star-forming regions visible. There are no signs of tidal tails or significant morphological distortions, indicating that the galaxy is likely not undergoing a major merger. There's some small evidence for possible minor disturbance of the galaxy, but it is quite dim.
