The galaxy presents a somewhat elliptical morphology. The central region displays a concentrated, bright, yellowish-white luminosity, suggesting a significant population of older stars. This luminosity diminishes gradually towards the outer regions. Faint, bluish regions are visible in the outer disk, possibly indicating areas of more recent star formation. There appears to be a slight asymmetry in the distribution of the outer regions, with a subtle extension visible on one side. No prominent spiral arm structures or a distinct bar are discernible in the image. The overall appearance is relatively smooth, suggesting a later-type galaxy that has largely exhausted its gas supply.
