The galaxy presents a smooth, centrally concentrated morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The color profile suggests a dominant population of older stars, exhibiting a yellowish hue characteristic of evolved stellar populations. The light distribution is generally round, with only slight deviations suggesting a deviation from perfect ellipticity. There is no strong evidence of ongoing major mergers or significant tidal disturbances. However, subtle asymmetries might indicate minor gravitational interactions in the past. Overall, the galaxy appears as an evolved system with a relatively quiescent star formation history.
