The galaxy presents a somewhat elliptical morphology. A central bulge is clearly visible, exhibiting a yellowish-white hue. Extending from the bulge are spiral arms, appearing predominantly bluish, suggesting the presence of younger, hotter stars. These arms are relatively tightly wound. There is no strong evidence of a bar structure bisecting the bulge. The disk is oriented at an oblique angle to our line of sight. The outer regions show some signs of tidal disturbances or irregular features, possibly indicating a past minor merging event. There is no particularly noticeable dust obscuration. The overall luminosity appears moderately high. The galaxy exhibits a moderately sized bulge in comparison to the disk size.
