The galaxy presents a largely smooth morphology. The light distribution appears relatively even, without prominent spiral arms or a well-defined disk structure. It appears nearly round, and lacks an elongated or cigar-like shape. There are no obvious signs of recent or ongoing major mergers or strong tidal disturbances. A minor disturbance may be indicated through slight asymmetries in the outer regions of the galaxy. The color profile suggests a slightly higher concentration of blue light towards the center, possibly indicating younger stellar populations in the core, while the outer regions show a redder hue.
