The galaxy presents as a relatively well-defined spiral galaxy with a moderate inclination relative to our line of sight. The central bulge appears prominent and exhibits a smooth, yellowish hue, suggesting an older stellar population. Two distinct spiral arms emerge from the core region. These arms show a clumpy structure, indicative of active star formation regions, which appear as brighter, bluer knots along the spiral structure. The arm structure shows a somewhat asymmetrical morphology, with one arm appearing more extended and developed than the other. Overall, the galaxy's color profile suggests a mix of stellar populations, with older stars in the bulge and ongoing star formation within the spiral arms. There are no obvious signs of major mergers or significant tidal disturbances, however there is some minor irregularity in the arm structure. The angular size is small.
