The galaxy presents a relatively smooth morphology, with a discernible, elongated shape. Its light distribution is concentrated towards the center, suggesting a prominent galactic nucleus or bulge. The overall color gradient transitions from a yellowish core to bluer peripheries. This may be indicative of older stellar populations dominating the central regions, and younger, hotter stars residing in the outer arms or disk, though distinct spiral arm structures are not apparent in this image. There is no strong evidence of ongoing major mergers or significant tidal disturbances. The galaxy exhibits a slight degree of asymmetry, hinting at a possible minor interaction or internal dynamic processes. 
