This galaxy appears to be a relatively undisturbed system at a redshift of approximately 0.167. Its morphology is largely smooth and elliptical, showing a high degree of central concentration. The galaxy exhibits a slight elongation, neither perfectly round nor distinctly cigar-shaped. There's no clear evidence of a disk component.

The galaxy's light distribution suggests an older stellar population, indicated by a redder color towards the core, suggesting a lower rate of recent star formation, although some bluer regions imply ongoing or recent star formation. There are no indications of major mergers or tidal disturbances. There may be some minor irregularities in the outer regions of the galaxy which could be minor disturbances.
