This galaxy appears as a relatively smooth, elliptical structure, with a high degree of central concentration. The color profile suggests a dominant population of older stars, exhibiting a reddish-golden hue overall. The galaxy lacks any distinct spiral arms or significant dust lanes. The morphology indicates it is likely a relatively massive system. The lack of blue light suggests a low rate of ongoing star formation. There is no immediately discernible evidence of any major merging activity or significant tidal disturbances.
