The galaxy presents a somewhat smooth morphology, with a slight central concentration of light. The overall shape appears to be elliptical, exhibiting a generally rounded profile, with no clearly defined spiral arms or prominent disk structures visible. There is faint color variation across the galaxy, suggestive of subtle differences in stellar populations or dust content. The galaxy does not appear to be undergoing a major merger, although there is a hint of possible minor disturbances in its outer regions. The light from the galaxy appears to be relatively uniform, suggesting an older stellar population. Given the overall characteristics, it's likely a moderately massive system with a modest star formation rate.
