The galaxy presents as a luminous, elongated structure with a high degree of central concentration. The color profile is dominated by blue wavelengths, suggesting a population of relatively young, hot stars and ongoing star formation. The overall morphology is suggestive of a highly flattened ellipsoidal shape, potentially exhibiting characteristics of a late-type spiral viewed edge-on or a lenticular galaxy. A faint, diffuse halo of lower surface brightness is visible surrounding the main body, extending further along the major axis. No distinct spiral arms or prominent dust lanes are discernible within the image, indicating a smoother distribution of stellar populations. There appears to be a slight warping in the isophotes, potentially indicating a mild gravitational interaction.
