The galaxy appears to be a spiral galaxy, observed at a slight incline relative to our line of sight. Definite spiral arm structures extend from a central bulge. These arms display a clumpy morphology, suggesting active regions of star formation. A faint bar structure may be present across the central bulge region. The galaxy is relatively isolated with no signs of any major interaction or disruption of its structure. The overall color of the galaxy suggests a mix of stellar populations, with bluer regions indicative of younger stars and redder regions likely populated by older stars. The light distribution appears centrally concentrated. The galaxy's disk extends a considerable distance.
