This galaxy, observed at a redshift of approximately 0.226, presents as an elliptical or lenticular system. The light distribution is relatively smooth and concentrated towards the center, exhibiting a yellow-orange hue suggesting an older stellar population. The galaxy appears elongated, with a cigar-like shape, and exhibits no discernible spiral arm structure or active star-forming regions. There is no evidence of a major merger or significant tidal disturbances affecting the system's overall morphology, although some minor disturbances may be present. The galaxy appears relatively quiescent, with a low rate of ongoing star formation.
