The galaxy appears to be a relatively smooth, elliptical galaxy, with a concentrated central bulge. The light profile suggests a fairly old stellar population, exhibiting a yellowish hue indicative of evolved stars. The overall shape is generally round. There's little evidence of spiral arms or significant dust lanes. A faint, extended halo of stars may be present, though the image resolution limits definitive confirmation. There do not appear to be any ongoing major merging events or significant tidal disturbances, suggesting that the galaxy is in a relatively relaxed state.
