The galaxy presents as a spiral type, viewed at a moderate angle relative to face-on. It exhibits two prominent spiral arms that emanate from a slightly elongated central bulge region. The arms display a somewhat flocculent structure, with discernible variations in surface brightness along their lengths, suggesting active star formation regions. Dust lanes appear interspersed within the spiral arms, particularly on the near side as defined by the tilt. The central bulge appears relatively small, suggesting it is either a small bulge or is simply not very luminous. The overall color of the galaxy indicates a mix of stellar populations, with bluer regions concentrated in the spiral arms implying ongoing star formation and redder hues dominating the central bulge, consistent with an older stellar population. There is no evidence of a strong bar feature. The galaxy shows signs of minor gravitational interaction, although the morphology is not significantly disturbed.
