The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. The central region is bright and concentrated, suggesting a prominent galactic nucleus. There is a lack of distinct spiral arm structure or a well-defined disk. Faint, diffuse extensions emanate from the central bulge, indicating a gradual decline in stellar density with increasing radial distance. Patches of redder light are visible in the galaxy. These areas may indicate regions of dust obscuration or ongoing star formation. There is no strong evidence of active galactic nuclei activity based on the lack of a highly luminous point source. Overall, the galaxy's features suggest a relatively quiescent system with a mature stellar population.
