The galaxy appears to be a spiral galaxy, exhibiting a prominent, centrally located bulge. The bulge displays a yellowish hue. The spiral arms are tightly wound, presenting a somewhat flocculent structure rather than a grand design. The arms themselves are bluer in color, suggestive of ongoing star formation activity. The galaxy's disk is not perfectly face-on, showing a slight inclination relative to the observer's line of sight. There is no readily apparent bar structure, but a degree of asymmetry is observed in the spiral arm distribution. The overall luminosity profile appears to be concentrated towards the center. There may be some minor tidal disturbances or evidence of a past or ongoing interaction.
