The galaxy appears as a fairly compact, luminous object with a centrally concentrated brightness profile. The overall color suggests a relatively evolved stellar population. The morphology seems predominantly smooth, with the light distribution appearing generally elliptical. There might be a very faint, diffuse halo extending beyond the main body of the galaxy, but the signal is weak. No distinct spiral arms or prominent dust lanes are visible. There is no evidence of active galactic nuclei activity. Based on its apparent size and redshift, it is likely a moderate-sized galaxy, possibly a lenticular or elliptical galaxy with a low rate of star formation. There are no signs of a major merger and appears to be undisturbed.
