The galaxy presents as a somewhat elliptical, luminous object with a central bulge. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population and a lower rate of star formation compared to the outer regions. Surrounding the central bulge, there's a more diffuse, bluish halo. The blue color indicates the presence of younger, hotter stars, implying ongoing or recent star formation within the galaxy's disk. The smoothness of the galaxy's overall structure indicates a relatively relaxed morphology, with no prominent spiral arms or significant tidal disturbances visible. However, some minor asymmetry is observed in the halo, potentially pointing towards past interactions or ongoing accretion events. The galaxy exhibits a moderate redshift, placing it at a significant cosmological distance.
