The galaxy presents an overall elliptical morphology, appearing somewhat elongated. A bright, concentrated central bulge is apparent, suggesting a significant population of older stars. Moving outward from the bulge, a fainter, more diffuse disk-like structure is discernible. The disk exhibits a bluer hue than the bulge, indicative of ongoing star formation. The galaxy lacks any clearly defined spiral arms, appearing largely smooth and featureless. There is a slight asymmetry to the outer regions of the disk, potentially suggesting minor gravitational interactions or past merger events. Overall, the galaxy appears to be an intermediate mass object with a relatively low rate of star formation.
