The galaxy presents as a somewhat elongated, elliptical-like structure. The light distribution is centrally concentrated with a bright core, suggesting a high density of stars in the galactic nucleus. The galaxy exhibits a smooth overall appearance, with no discernible spiral arms or prominent dust lanes visible at this resolution. The color gradient appears to transition from a yellowish hue at the core to slightly redder tones in the outer regions, potentially indicating older stellar populations further from the center. There seems to be another possible object close to the galaxy, potentially a neighboring galaxy that looks to be less defined than the main galaxy. The image quality limits the ability to identify finer details of the galactic morphology and stellar composition. Overall, based on visual inspection, the galaxy seems to be a relatively massive galaxy with little active star formation and with a likely companion galaxy.
