The galaxy appears to be a spiral galaxy, presenting a near face-on orientation. Two to three prominent spiral arms emerge from a bright central bulge. The arms exhibit a somewhat flocculent structure, showing localized regions of increased luminosity, suggestive of active star formation. The bulge dominates the inner region of the galaxy, with light that is yellowish-white in color. The spiral arms show bluer tints than the bulge region. A weak bar may be present across the bulge. The spiral arms seem to be somewhat tightly wound. There does not appear to be any indications of recent or ongoing major merger events.
