The galaxy presents as a somewhat elliptical structure, with a bright, concentrated central bulge region that emits strongly in the yellow. This suggests a substantial population of older stars in the galactic nucleus. Fainter, diffuse blue light emanates from the outer regions, possibly indicating ongoing star formation, or the presence of a younger stellar population. The galaxy does not exhibit strong spiral arm features or a well-defined disk structure from this angle, but there is some blue, less concentrated structure on either end. The overall morphology suggests a galaxy somewhere between a pure elliptical and a spiral galaxy, possibly an S0 type. There's no clear indication of any major merger events or significant tidal disturbances.
