The galaxy presents as a lenticular or early-type spiral, exhibiting a generally smooth morphology with a subtle disk component. The central bulge is bright and concentrated, with a yellowish hue, indicative of an older stellar population. A faint, diffuse disk extends outwards from the bulge, appearing somewhat flattened. There is little evidence of distinct spiral arms or active star formation regions within the disk; its color is a mix of yellowish hues with a slight bluing toward the outer edges, suggesting a moderate amount of younger stars. A small amount of disturbance in the structure is seen, and the overall shape is neither perfectly round nor elongated, showing a relatively round morphology, which implies it is more likely an early-type spiral, or a lenticular galaxy transitioning from a spiral to an elliptical morphology.
