The galaxy presents as a somewhat disturbed system, exhibiting characteristics suggesting an ongoing or recent merger event. The morphology is neither purely elliptical nor spiral, but displays features of both. There is an overall elongated shape. The central bulge appears present, but not particularly bright, suggesting a moderate stellar population density. Faint hints of possible tidal features or disrupted arms are visible, further suggesting an interaction.

Color gradients within the galaxy indicate varying stellar populations. There appears to be a general bluer tint indicating ongoing star formation in the region. A distinct feature is its distorted overall appearance, indicative of gravitational interaction or recent merger. The morphology doesn't fit neatly into standard galaxy classifications, hinting at a system undergoing significant evolutionary changes.
