The galaxy presents as a moderately luminous object with an overall elliptical morphology. It exhibits a smooth appearance with a centrally concentrated bulge.  The galaxy shows a slight elongation, deviating from a perfect circle. Faint blue tinges are visible in the surrounding disk indicating modest amounts of on-going star formation. There is some evidence of minor disturbances within the galaxy, possibly due to a recent interaction or merger. The core is significantly brighter than the outer regions, exhibiting a yellowish hue indicative of an older stellar population concentrated in the center. Overall, this appears to be an intermediate-mass galaxy undergoing minor disturbances.
