The galaxy presents as a moderately sized, lenticular or early-type spiral galaxy at a redshift of approximately 0.087. Its morphology is characterized by a dominant, smooth central bulge that exhibits a yellowish hue, indicative of an older stellar population. The light distribution appears centrally concentrated with a gradual decline in surface brightness moving outwards. Evidence of a distinct disk component is subtle, suggesting a relatively smooth, featureless structure with minimal signs of spiral arms or active star formation. The overall shape is generally elliptical, but not perfectly round, with a slight elongation. There is no apparent ongoing major merger activity, but potentially hints of minor tidal disturbances or interactions may be present. The galaxy exhibits intermediate color indices, with DESI magnitudes showing a redder color in g-r and r-z bands suggesting intermediate star formation rates. Overall, the galaxy appears to be a relatively quiescent system with a moderately sized stellar mass.
