The subject galaxy presents as an elongated, disk-shaped system. Its structure appears to be largely featureless, exhibiting a relatively smooth light distribution. The color profile suggests the presence of an older stellar population, with a general blue hue. There's some color variation at the edges of the galaxy. The disk appears to be near edge-on, lacking a prominent central bulge. No significant spiral arm structure or dust lanes are readily apparent. The galaxy exhibits a low level of star formation activity, based on the galaxy's color and lack of prominent HII regions. There may be some faint tidal disturbances or signs of past interactions in the galaxy's outer regions, but it is largely undisturbed. The galaxy is relatively small. There is no evidence of a recent major merger event.
