The galaxy appears as a centrally concentrated object with a generally smooth morphology. It presents a largely elliptical shape, exhibiting a high degree of central luminosity that diminishes gradually outwards.  The light distribution suggests a well-established, mature stellar population. The galaxy's color profile indicates the presence of both older, redder stars and younger, bluer stars, with the concentration of bluer stars being in the central area. There may be a very small tidal tail on the left side, indicating past or recent merger events. There is no obvious active galactic nucleus or dust lane visible in the image. Overall, the galaxy appears to be a relatively quiescent, massive galaxy.
