The galaxy presents an overall elliptical morphology. The light distribution indicates a central bulge region with a fairly uniform brightness distribution. It is a relatively smooth distribution, with no obvious spiral arm structures are visible. The galaxy's shape exhibits a near-circular, almost lenticular appearance. There is a relatively faint outer halo surrounding the central region, this halo appears diffuse and extended. Embedded within the central bulge are several patches of distinct color variations and irregular morphology. These may be indicative of ongoing star formation. Overall, there appears to be evidence of minor disturbances and activity, though the galaxy remains relatively stable in overall structure.
