The galaxy presents a predominantly smooth, rounded morphology, exhibiting a central concentration of light suggestive of a prominent bulge. There's a slight elongation visible, though overall, it appears largely spheroidal. The color gradient suggests a stellar population dominated by older stars, evidenced by the reddish hues at the core and periphery, with possibly some younger stars concentrated towards the central region, where a slightly bluer tone is observed. No distinct spiral arms or disk features are discernible. There are no obvious signs of ongoing major merger activity or significant tidal disturbances in its immediate vicinity. Based on the characteristics observed, the galaxy appears to be a relatively massive system with little star formation occurring.
