The galaxy presents a generally smooth morphology, appearing somewhat elongated or cigar-shaped. A central bulge region is discernible, exhibiting a concentrated luminosity gradient compared to the outer regions. The galaxy displays a color profile indicative of an older stellar population; the central region shows a yellowish hue that may represent more evolved stars. There appears to be a small, almost imperceptible hint of a disk structure, but it is difficult to tell. It is likely that star formation is suppressed in the galaxy. No significant tidal disturbances or signs of merging activity are evident in this image.
