The galaxy presents as a relatively compact, elliptical structure. Its central region exhibits a bright, concentrated core, suggesting a high density of stars. Moving outward, the luminosity gradually decreases, with no distinct spiral arms or prominent disk-like features visible. 

The overall color appears slightly redder, indicative of an older stellar population and a lower rate of star formation. There may be a trace amount of irregular distribution in the light, perhaps caused by a small disturbance. The galaxy's shape tends toward a round morphology. The shape could also suggest a face on galaxy as well.
