The galaxy presents as a moderately bright, slightly elongated structure. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus or bulge. The colour appears to be largely homogenous with a slightly yellowish hue, this may indicate the presence of an older stellar population. Faint, diffuse outer regions are visible, extending outwards from the core and indicating the presence of a disk structure. There are no readily discernible spiral arm structures. No major signs of galactic interaction are noted, such as tidal tails or distorted morphology. The galaxy appears to be relatively undisturbed.
