The object presents as a faint, diffuse source with an elongated morphology. There appears to be a subtle central concentration, but the overall light distribution is relatively smooth and lacks distinct spiral arm features. There are no apparent dust lanes or significant star-forming regions visible. A possible minor disturbance in the morphology of the galaxy is visible, but without a clearer image, it's difficult to determine whether this is the result of an ongoing or past minor merger event. The color profile suggests a higher proportion of redder stellar populations and a lack of significant recent star formation activity.
