The galaxy presents as a relatively faint, disk-shaped system, viewed nearly edge-on. A central bulge is visible, appearing more concentrated and possessing a yellowish hue, suggesting an older stellar population. The disk component extends outwards, exhibiting a bluer color, which may indicate the presence of younger, hotter stars and ongoing star formation. The disk appears relatively smooth with limited signs of strong spiral arm structures. The overall morphology suggests the galaxy is an inclined disk galaxy, possibly of a later type, though the lack of distinct spiral features may point towards a lenticular classification. No significant tidal disturbances or interacting companions are readily apparent, indicating the galaxy has likely not undergone a major merger recently.
