The galaxy presents as a centrally concentrated object with a generally smooth morphology. It appears roughly elliptical in shape, exhibiting a high degree of roundness. The core region displays a yellowish hue, suggesting an older stellar population. Fainter, bluer light is observed in the outer regions of the galaxy, indicative of more recent star formation relative to the core. There is no discernible spiral structure or prominent dust lanes visible in this image, and it doesn't appear to be undergoing any major merger events or significant tidal disturbances. The overall luminosity suggests a massive galaxy.
