The galaxy presents as an elongated, elliptical structure. Its overall color profile appears to be redder, suggesting an older stellar population. The light distribution is relatively smooth, with no discernible spiral arms or prominent dust lanes visible. There is a slight concentration of luminosity towards the center of the galaxy, suggesting a central bulge or core. The outer regions of the galaxy fade gradually into the background, indicating a diffuse halo. There appears to be no significant ongoing star formation within the galaxy. There is no visual evidence of any tidal disturbances or interactions with neighboring galaxies. The general morphology suggests a passively evolving system, likely a lenticular or elliptical galaxy viewed at an oblique angle.
