The galaxy presents as a relatively well-defined spiral structure. The spiral arms appear somewhat flocculent, lacking strong definition, but are still clearly visible extending from a central bulge region. The bulge appears moderately prominent and is characterized by a yellowish hue, suggesting an older stellar population. The spiral arms exhibit a bluer tint, indicative of ongoing star formation and a younger stellar population. The galaxy appears to be viewed at a slight angle, showing moderate inclination. No obvious bar structure is discernible in the central region. No major signs of active galactic nuclei are visible, such as extended jet structures. Evidence of minor disturbances is hinted at by a slight asymmetry in the distribution of light within the spiral arms, although a major ongoing merger is unlikely. The overall morphology suggests a spiral galaxy type, possibly with characteristics of both early and late-type spirals.
