The galaxy presents as a late-type spiral, though the spiral arm structure is not strongly defined. A dominant, moderately sized bulge is visible, exhibiting a yellowish hue that suggests an older stellar population. The disk of the galaxy, surrounding the bulge, shows a bluer color, possibly indicating ongoing star formation. There may be some degree of tidal disruption of the galaxy. The galaxy's orientation appears to be inclined relative to our line of sight, offering a partial view of its disk. Overall the galaxy has a relatively smooth appearance.
