The galaxy presents as an elongated, disk-like structure viewed at a significant inclination to our line of sight. The central region exhibits a bright, concentrated luminosity suggesting a well-defined nucleus or bulge. The color gradient transitions from a bluer hue in the central region to a more neutral, possibly redder, tone in the outer regions of the disk. This color shift may indicate variations in stellar populations, with younger, bluer stars dominating the central regions and older, redder stars residing in the outer disk. The outer edges of the disk appear somewhat diffuse and irregular, lacking distinct spiral arm structures. This suggests the galaxy may be an early-type spiral or a lenticular galaxy with a relatively smooth stellar distribution. There is little evidence of significant dust lanes or active star formation regions visible in this image. The overall morphology suggests a relatively quiescent galaxy with a moderate stellar mass and low star formation rate.
