The galaxy presents a predominantly smooth morphology, suggesting a classification as an elliptical galaxy. The light distribution is concentrated towards the center, with a gradual decrease in brightness towards the outer regions. There is a slight deviation from perfect circularity; the galaxy appears somewhat elongated along one axis. The color profile exhibits a redder hue overall, indicative of an older stellar population and lower ongoing star formation activity. There is only minimal evidence of any distinct structural features such as spiral arms or a well-defined dust lane. There is a very slight hint of a faint halo, and a potential minor tidal disturbance, but further investigation is needed to support this. Based on its size and brightness, this appears to be a galaxy with a substantial stellar mass.
