The galaxy appears to be a spiral, seen at a significant angle relative to our line of sight. This orientation obscures a full view of the spiral arm structure, although hints of a disk are visible. The central bulge appears prominent and relatively bright, suggesting a significant population of older stars and possibly a supermassive black hole actively accreting material. The galaxy exhibits a generally smooth appearance, with only subtle irregularities in its shape. The overall color is yellowish-white, indicating a mix of stellar populations but suggesting a lack of significant ongoing star formation. There's a slight asymmetry in the disk, possibly hinting at a minor gravitational interaction or past merger event, though no significant tidal features are readily apparent. The edges of the galaxy seem somewhat diffuse, making it challenging to precisely determine its overall size and shape.
