The galaxy appears as a relatively small, elliptical or lenticular system at a redshift of approximately 0.245. It exhibits a generally smooth morphology with a high degree of roundness and radial symmetry, showing a lack of prominent spiral arms or a distinct central bar structure. The galaxy's color profile suggests it is comprised mainly of older stellar populations and a low ongoing star formation rate. There is little evidence of significant dust lanes or patchy star-forming regions. There are no strong indications of ongoing major merger activity or tidal disturbances, but slight irregularities in the outer isophotes may suggest a minor interaction in the recent past.
