The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light profile. The core exhibits a yellowish hue, suggestive of an older stellar population. Proceeding outwards, a faint bluish halo surrounds the core, possibly indicative of some ongoing, albeit low-level, star formation. The shape is generally rounded, exhibiting a slight elongation that gives it a somewhat cigar-shaped appearance. No significant tidal features or signs of major mergers are readily apparent, though a subtle disturbance cannot be entirely ruled out. The galaxy appears as a relatively isolated system in this field.
