The galaxy presents as a spiral galaxy with a redshift of approximately 0.124. Its overall form is moderately inclined relative to our line of sight. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. Faint spiral arms emanate from the bulge, extending outwards, displaying a bluer color, indicative of more recent star formation. The arms are moderately wound and somewhat fragmented. The galaxy exhibits a relatively high level of overall symmetry. No strong bar structure is apparent. No obvious signs of a major merger event are visible. The galaxy's estimated effective radius is a few kiloparsecs. Overall mass is estimated to be approximately 10^10.5 solar masses and has ongoing star formation happening within it.
