This galaxy presents a morphology suggestive of a spiral galaxy viewed at a significant inclination. The central region exhibits a bright, concentrated bulge, characterized by a yellowish hue, indicative of an older stellar population and potentially higher metallicity. Extending outwards from the bulge, there's evidence of a faint, bluer disk. Although there are no distinct spiral arms visible, the bluish tint suggests the presence of younger, hotter stars and ongoing star formation within the disk component. There is some evidence of possible minor disturbance/merging activity to the top of the galaxy. The galaxy's overall shape appears somewhat elongated, with the estimated size of the galaxy being approximately 7 kpc.
