The galaxy presents as a face-on spiral with relatively loose, well-defined spiral arms. Two main arms are particularly prominent, extending from a moderately sized central bulge. The spiral arms exhibit a clumpy structure, suggesting active star formation regions. The central bulge appears yellowish, potentially indicating an older stellar population. The arms show a mix of blue and reddish hues, with the bluer regions likely corresponding to younger, hotter stars and the redder regions potentially indicating the presence of dust or older stellar populations. There is no obvious bar structure. There may be signs of minor tidal disturbances or interactions given the slight asymmetry in the arm structure, but no major merger event is apparent. Overall, the galaxy seems to be a relatively well-formed spiral galaxy with ongoing star formation.
