The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. The light distribution suggests a roughly spheroidal shape, with a high degree of symmetry. A slight elongation is present but does not disrupt the overall rounded appearance.

The color profile indicates an older stellar population, predominantly characterized by yellow and reddish hues. The central region exhibits the most concentrated light, gradually fading toward the outer edges. There's little evidence of distinct spiral arms or prominent dust lanes. The overall structure suggests that the galaxy is relatively evolved, with a quiescent or slowly declining rate of star formation. Minor disturbances may be present, however no major mergers appear to be actively occurring.
