The galaxy presents as a highly inclined disk galaxy, likely seen nearly edge-on. A prominent central bulge is visible, appearing somewhat rounded. The galaxy exhibits a relatively smooth texture, suggesting a lack of significant spiral arm structure or prominent star-forming regions. There is no evidence of a major merger or significant tidal disturbances. There is some indication of minor disturbance. Overall, the galaxy is estimated to be of moderate mass, with indications of active but not excessive ongoing star formation.
