The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core exhibits a yellowish hue, potentially indicating a population of older stars. There is a subtle gradient in color moving outwards from the center towards the edge of the galaxy, becoming slightly redder. This could be indicative of changes in the stellar population or dust content. The galaxy does not appear to have significant spiral arms or a prominent disk. Based on its shape, it may be more of an elliptical morphology. No signs of major mergers or significant tidal disturbances are visible. The relatively smooth, symmetrical appearance suggests it is a settled system.
