The object presents as a spiral galaxy, seen at a slight angle relative to face-on. The galactic nucleus exhibits a yellowish hue, possibly indicative of an older stellar population or dust obscuration. Two spiral arms are readily discernible, tracing a somewhat symmetrical pattern outward from the central bulge. The winding of the spiral arms appears to be moderate, neither tightly wound nor extremely loose. There appears to be a bar structure, but it is difficult to make out due to the distance of the galaxy from the observer. The galaxy displays relatively low merger activity. The apparent color gradient suggests potential ongoing star formation within the spiral arms, exhibiting a bluer tinge compared to the central region. Overall, the galaxy appears to be a well-defined, moderately active spiral system.
