This galaxy exhibits a morphology consistent with a spiral type, presenting a notable disk structure. Evident spiral arms emanate from a somewhat prominent central bulge. These arms appear loosely wound. The galaxy's orientation is inclined relative to our line of sight. There appears to be a possible bar structure. The light distribution suggests a significant population of older stars within the central bulge, indicated by the redder hue, while the disk component shows bluer colors, possibly indicating ongoing star formation. The galaxy displays features associated with relatively minimal disturbances.
