The galaxy presents with an apparent angular size that suggests it is not overly distant, enabling observation of morphological details. It appears to be a spiral galaxy, displaying a mixture of smooth and featured characteristics. The central bulge exhibits a yellowish hue, indicative of an older stellar population, likely dominated by red giants and older main sequence stars.

Moving outward from the bulge, evidence of spiral arms is present, though not highly defined. The arms display a bluer color compared to the bulge, which is consistent with ongoing star formation activity, indicated by younger, hotter stars and HII regions. There is a slight asymmetry or disturbance in the overall structure, perhaps indicating a past or ongoing interaction. This distortion appears most prominent in the outer regions of the disk. The galaxy is presented in a face on configuration.
