The galaxy presents as a spiral type, with a relatively bright central bulge exhibiting a yellowish hue, indicative of an older stellar population.  Spiral arms are clearly visible and quite prominent, tightly wound and extending outwards from the bulge. These arms display a bluish tint, implying the presence of younger, hotter stars and ongoing star formation. The morphology suggests a classification towards the later end of the spiral sequence, possibly type Sc, due to the prominent, open spiral arms. There is some asymmetry visible, with more prominent spiral structure on one side of the bulge than the other. This could imply minor gravitational interactions or a lopsided distribution of gas and dust within the disk. No obvious signs of strong bars or major merger events are seen.
