This galaxy presents as an elongated, disk-shaped system, likely a spiral galaxy viewed at a moderate inclination. A bright, concentrated central bulge is clearly visible, exhibiting a yellowish-white hue indicative of an older stellar population. The disk component appears less defined, showing a mottled texture with hints of spiral arm structures. The color of the disk is generally bluer than the bulge, suggesting the presence of younger, hotter stars and ongoing star formation. The overall morphology suggests a galaxy that is neither perfectly smooth nor highly disturbed, with possible minor interactions.
