This galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution. A slight elongation is visible, suggesting it is not perfectly spherical. The central region appears brighter and more compact, indicating a higher concentration of stellar mass and possibly a supermassive black hole. 

The overall color profile of the galaxy suggests an older stellar population, with a greater proportion of redder stars compared to bluer, younger stars typically found in spiral arms. There are subtle asymmetries in the outer regions of the galaxy, which could be indicative of past minor merging activity or gravitational interactions with nearby galaxies. No distinct spiral arms or prominent dust lanes are apparent. Overall, the galaxy appears relatively undisturbed.
