The galaxy exhibits a spiral morphology, presenting a prominent disk structure. The spiral arms are well-defined, tracing a pattern suggestive of a grand design spiral, primarily composed of two arms. These arms are moderately wound. The central bulge is notable, appearing neither overly dominant nor negligible in size, contributing significantly to the overall luminosity. The galaxy appears undisturbed, without any obvious signs of merging or tidal interactions. There is no visible stellar bar. The overall color index suggests a mix of stellar populations, with bluer hues apparent along the spiral arms, potentially indicating regions of active star formation. The redder colors around the bulge may be due to an older, more evolved stellar population.
