This galaxy presents as a spiral type, observed at a moderate inclination angle. It is characterized by prominent spiral arms that extend from a central bulge region. The spiral arms appear well-defined, suggesting a structured and dynamically stable configuration. These arms exhibit a bluer hue, indicative of ongoing star formation activity and the presence of younger, hotter stellar populations within these regions.

The central bulge region is relatively bright and appears yellowish in color, suggesting an older stellar population that is largely devoid of active star formation. No strong bar structure is visible traversing the central region. The galaxy displays a generally symmetrical morphology, though there are hints of some minor disturbance or asymmetry in the outer arms. Overall, the galaxy appears relatively isolated and does not exhibit clear evidence of ongoing or recent major merger events. The estimated size suggests a relatively substantial, though not exceptionally large, spiral galaxy.
