The galaxy presents as a generally smooth, elongated elliptical galaxy with a cigar-like shape. A bright, somewhat amorphous central bulge is observed, with a reddish hue suggestive of an older stellar population. Extending outward from the core, the galaxy displays a fainter, more diffuse halo. This halo appears bluer in color, hinting at some regions of more recent star formation. There is no indication of strong spiral arm structure, although slight irregularities in the halo's color distribution might suggest minor tidal disturbances or ongoing minor merger events. Overall, the galaxy appears relatively isolated and undisturbed.
