The galaxy presents a roughly elliptical morphology, though some asymmetry is visible. A central bulge is apparent, exhibiting a higher concentration of light. Faint spiral arm structures appear to emanate from this central region, though they are not sharply defined and show patchy areas of star formation. The overall color suggests a population of both older, redder stars and younger, bluer stars, with the bluer stars possibly concentrated in the spiral arms. Indications of a minor disturbance are suggested by some irregularities in the outer regions of the galaxy. The galaxy is relatively small, occupying a limited angular extent in the image. The apparent smoothness in some regions alongside the disk features and subtle disturbances suggests that the galaxy may be undergoing or has recently undergone some form of interaction or minor merger. The system exhibits a moderate degree of dust obscuration.
