This galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The bulge exhibits a yellowish hue, suggesting a population of older, redder stars. Fainter, bluer light is observed emanating from what appear to be spiral arms extending from the central bulge. These arms are not well-defined, lending the galaxy a somewhat diffuse and flocculent appearance. There's a slight asymmetry to the galaxy's overall shape, hinting at possible past interaction or internal disturbances. The relatively smooth appearance of the disk implies a relatively low current star formation rate.
