The galaxy presents as an inclined spiral, exhibiting a moderate degree of central concentration. The core region shows a yellowish hue, possibly indicative of an older stellar population. Faint, elongated arms extend from the central region, appearing somewhat disrupted or flocculent in structure. These arms display a bluer tint, suggesting the presence of younger, hotter stars. There is a slight asymmetry in the distribution of light within the arms. The overall color profile suggests a mixture of stellar populations. There appears to be a slight central bulge but not very pronounced. There is no obvious dust lane present in the image.
