The galaxy presents a generally smooth appearance, with a concentrated central bulge dominating the overall structure. The morphology is relatively round, exhibiting a slight ellipticity but lacking any prominent disk-like features or spiral arms discernable from this imagery. The core is notably luminous, indicating a high concentration of stars and/or an active galactic nucleus, emitting strongly in g, r and z bands. There's little evidence of significant dust lanes or complex structures within the galaxy's body. The colour profile suggests a population of relatively older stars, contributing to the yellowish hue. There appears to be no ongoing major merger activity or significant tidal disturbances affecting the galaxy's structure.
