The galaxy appears to be an elliptical or lenticular galaxy at a moderate redshift, approximately 0.24. It is relatively compact, with an estimated effective radius around 6.5 kpc. The galaxy presents a smooth, largely featureless morphology. There is little evidence of spiral arms or prominent dust lanes. The galaxy exhibits a concentration of older stellar populations, as evidenced by the redder color indices. Star formation is present, but appears to be subdued, indicative of a low specific star formation rate. No major mergers or significant tidal disturbances are immediately obvious, but the possibility of minor interactions cannot be ruled out. The overall structure is generally round, showing no strong elongation or signs of major asymmetry.
