The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth morphology with a general elliptical shape. A slight elongation is observable along a rough horizontal axis. The galaxy's color profile shows a predominantly yellowish-white core, likely indicative of an older stellar population. There is a hint of redder hues at the galaxy's periphery, suggestive of possible ongoing star formation in the outer regions or simply an area with a higher abundance of dust attenuating the bluer light from young stars. There are some slight possible signs of tidal disturbance in the red area. Overall, the galaxy appears to be a massive system with a stellar mass in the higher ranges.