The galaxy presents as a slightly inclined, disk-like structure, approximately 3.4 kpc in radius. The color profile suggests a prominent central bulge that appears relatively smooth and exhibits a yellowish hue, indicative of an older stellar population with lower ongoing star formation activity. A fainter, bluer disk component is observed, extending outwards from the bulge and towards the right, suggesting the presence of younger stars and some ongoing star formation. There are hints of mild disturbances in the disk, though the overall morphology is mostly undisturbed. The galaxy appears relatively massive and displays a relatively low rate of star formation.
