The galaxy appears as a somewhat elliptical, diffuse object with a concentrated central bulge. Its color profile indicates an older stellar population, dominated by yellowish hues, with some redder regions possibly indicating dust absorption or older stars. There is little evidence of distinct spiral arm structures or significant recent star formation activity. The smoothness of its light distribution suggests a galaxy that has largely settled into a stable configuration, with no ongoing major mergers, or tidal disturbances immediately visible.
