The galaxy presents a morphology that appears predominantly smooth, with a concentrated central region exhibiting a bright, intense light profile. Faint, diffuse extensions are discernible around this core, giving the impression of a more extended body. Overall shape looks rather lenticular. There are no clear spiral arm structures or dust lanes visible in this image. There may be some minor disturbances or a possible interaction with a smaller object nearby, evidenced by slight asymmetries in the outer halo. The central brightness indicates a concentration of older stars, but is not bright enough to indicate active galactic nuclei. The light from the galaxy is slightly shifted towards the redder end of the spectrum indicating that the galaxy is relatively old and has low to moderate levels of star formation. 
