The galaxy presents as a moderately inclined disk system. It has a concentrated central bulge that blends smoothly into the surrounding disk. The overall color is a bluish-white hue, indicating the presence of a substantial population of young, hot stars. The morphology suggests a relatively evolved system, with a smooth light distribution and no obvious spiral arm structures visible at this resolution. The light distribution is centrally concentrated. The elongation of the galaxy is prominent, with an axis ratio suggesting a somewhat flattened structure. There appears to be a faint degree of disturbance in the disk, possibly due to minor tidal interactions or internal dynamical processes.
