The galaxy presents as an elliptical morphology, exhibiting a predominantly smooth structure with a slight elongation. The central region displays a concentrated luminosity, suggesting a dense stellar population, potentially an older population based on the yellow color. The light becomes more diffuse towards the outer regions of the galaxy, but not many distinct features are visible. There is minimal evidence of spiral arms or prominent dust lanes; although, a potential disturbance in the galaxy, given its non-circular shape, cannot be completely ruled out. The overall color profile indicates relatively low star formation activity.
