The galaxy presents a generally smooth morphology, exhibiting a concentrated central bulge that fades into a less defined surrounding halo. The color profile shows a reddish-orange core, suggesting an older stellar population dominating the central region. A subtle gradient towards bluer hues is observed in the outer regions of the halo, indicative of possible ongoing or recent star formation activity at a relatively low rate. The galaxy appears relatively isolated, showing no obvious signs of major mergers or significant tidal disturbances, although there's a minor hint of asymmetry in the outer halo. It does not show a well defined disk. The galaxy is moderately luminous. Its estimated size is compact.
