The galaxy presents an overall smooth and rounded morphology, with a high degree of central concentration. The light profile appears relatively featureless, exhibiting a gradual decline in intensity from the bright core outwards. No distinct spiral arms or bar structures are discernible. Color gradients are subtle, with a slightly bluer hue present in the outer regions compared to the central bulge, which appears more yellow and red. There is no evidence of a major ongoing merger, but a potential minor disturbance cannot be fully excluded. The galaxy exhibits a moderate redshift, and based on estimated magnitudes and overall appearance, this galaxy likely has a stellar mass on the order of 10^10 solar masses. There is a low level of star formation activity. The estimated effective radius indicates that this is a relatively compact galaxy.
