The galaxy presents as a spiral, viewed at a significant angle relative to face-on. The central bulge appears moderately prominent and exhibits a yellowish hue, suggesting an older stellar population. Faint spiral arms are visible extending from the bulge, tracing a relatively open winding pattern. A strong bar structure traverses the central region. The disk component displays a mottled texture, indicative of star-forming regions, though these are not sharply defined, suggesting a moderate amount of star formation is occurring. There are some hints of disturbances that may be caused by minor gravitational interactions with another galaxy. The galaxy appears to be relatively isolated in its immediate vicinity.
