The galaxy presents as a moderately bright, elliptical or lenticular structure with a concentrated central bulge. The core exhibits a yellow-orange hue, indicative of an older stellar population. A slightly flattened disk component may be present, although it is not strongly defined. There appears to be little to no evidence of strong spiral arm structure. The overall morphology suggests a relatively smooth appearance, with a slight elongation observed. No significant signs of recent or ongoing major mergers or tidal disturbances are immediately apparent. The galaxy exhibits a redshift indicating that it is a fairly distant object. The mass of the galaxy is quite large, with a small star formation rate. The average light detected is slightly lower in the G band compared to the R and Z bands.
