The galaxy presents a generally smooth morphology, with a central bulge that appears slightly elongated. The overall shape resembles a flattened spheroid, transitioning towards a cigar-like appearance. The central region is characterized by a concentration of light, suggestive of an older stellar population. Moving outwards from the core, a faint disk-like structure is barely visible, exhibiting a subtle bluish tint, hinting at the presence of younger, star-forming regions. There are no clear signs of spiral arms or strong irregularities. The galaxy may be undergoing some form of minor interaction, indicated by slight disturbances in its overall structure. Overall, the galaxy appears to be a massive system, transitioning from an active star-forming phase to a more quiescent state.
