The galaxy appears as a moderately bright, somewhat elongated object with a smooth, diffuse structure. The core region exhibits a yellowish hue, possibly indicating a higher concentration of older stellar populations. Moving outward from the core, the color transitions to a slightly bluer tone, suggestive of some ongoing, albeit limited, star formation activity. The galaxy does not show any clear spiral arm structure or a well-defined disk. There may be some minor tidal disturbances. Overall, the galaxy appears to be a relatively evolved system with a dominant spheroidal component and subdued star formation.
