The galaxy presents as a barred spiral, with tightly wound spiral arms. The central bulge appears to be of moderate size and exhibits a yellowish hue, likely indicative of an older stellar population. The spiral arms are not well-defined, and the disk is the dominant feature. There is no indication of any major ongoing merger activity, though minor disturbances or interactions cannot be ruled out. The galaxy's color suggests it is likely a relatively quiescent galaxy with modest star formation.
