The galaxy presents as a spiral type, exhibiting a moderately inclined disk relative to our line of sight. A central bulge is present, characterized by a yellowish-orange hue, suggesting an older stellar population. Faint spiral arms emanate from the central bulge, loosely wound and somewhat indistinct. These arms display hints of bluer regions, indicating areas of recent or ongoing star formation. The dust lanes in the spiral arms are not very pronounced, giving them a somewhat fuzzy appearance. Overall, the galaxy shows no obvious signs of major interactions or mergers, although a subtle distortion in one of the outer arms cannot be ruled out as a possible minor disturbance.
