The galaxy presents as a relatively smooth, elliptical structure, exhibiting a notable lack of distinct spiral arms or features indicative of active star formation regions. The light distribution is concentrated towards the galactic center, suggesting a high stellar density in the core. The galaxy's color profile indicates a population of older stars, potentially dominated by redder giants. There's little evidence of recent or ongoing major mergers, though minor tidal disturbances cannot be ruled out. The overall morphology suggests a system approaching quiescence, with a low specific star formation rate relative to its mass.
