The galaxy presents as a generally smooth structure with an elliptical morphology. A bright, concentrated central bulge is evident, exhibiting a yellowish-orange hue, suggesting an older stellar population. The bulge dominates the galaxy's overall luminosity. Surrounding the bulge, a fainter, more diffuse disk component can be observed. The disk appears relatively featureless, lacking prominent spiral arms or dust lanes. The disk color appears bluer than the bulge, indicative of the presence of younger, hotter stars and perhaps ongoing star formation. There appears to be little to no evidence of major mergers or tidal disturbances in the galaxy's morphology, though some minor asymmetry is noted. The galaxy exhibits a moderate degree of redshift, indicating that it is at a significant cosmological distance.
