The galaxy presents a generally smooth, elliptical morphology, appearing more rounded than elongated. There is a concentrated central bulge, exhibiting a yellowish hue suggestive of an older stellar population. Surrounding the core, a faint disk-like structure is observed, subtly inclined relative to our line of sight. The outer regions of the galaxy gradually fade into the background, indicating a diffuse halo. No prominent spiral arms or significant dust lanes are discernible in this image, nor are any obvious signs of recent major merger activity or tidal disturbances apparent, although there may be some minor disturbances. The galaxy's overall color profile suggests a relatively low ongoing star formation rate.
