The galaxy presents as a relatively smooth, elliptical morphology, with a central bulge that appears quite luminous. The concentration of light is highest at the nucleus, decreasing gradually towards the outer regions. Faint hints of a disk structure may be present, but it is not a dominant feature. There appears to be some minor disturbance or interaction occurring, as evidenced by slight asymmetries or irregularities in the galaxy's shape. Overall, the galaxy lacks strong spiral arms or prominent star-forming regions. The color distribution is predominantly redder, suggesting an older stellar population and relatively low star formation activity.
