The galaxy presents a largely smooth and rounded morphology. There is a central bright region, which is likely the galactic bulge. The color of this central region appears somewhat redder, suggesting an older stellar population. Surrounding the bulge is a fainter disk component, which appears bluer, hinting at ongoing star formation. However, the overall smooth appearance suggests a limited amount of recent or current star formation. There is no obvious spiral structure or significant dust lanes visible in the image. The galaxy does not appear to be undergoing any major merging activity. Faint asymmetrical extensions are visible, which could be tidal streams, and indicate a potential minor interaction with another galaxy in the distant past.
