The galaxy presents as a smooth, elliptical structure, elongated in shape. A concentrated central bulge is observed, exhibiting a yellowish-white hue suggestive of an older stellar population. Moving outwards from the core, the galaxy smoothly transitions to a fainter, bluer halo. No distinct spiral arm structures are discernible. The overall morphology suggests a relatively evolved system, with low ongoing star formation. Subtle distortions or tidal features are not readily apparent, indicating that the galaxy is likely undisturbed and not undergoing any significant merging activity. The elongated form indicates that it may be observed as a cigar shape.
