The observed galaxy exhibits a generally smooth morphology. It appears nearly round. There is little visual evidence of spiral arms or a prominent disk structure. The galaxy displays a concentrated central bulge. The light profile suggests a relatively evolved system. While the majority of its light emanates from older stellar populations, some ongoing star formation cannot be ruled out. There is minimal indication of any recent or ongoing major mergers or significant tidal disturbances. The galaxy appears relatively isolated, without any obvious companions.
