The galaxy appears to be a disk galaxy, viewed at a steep inclination, resulting in a flattened, elongated shape. A bulge is not easily discernible, suggesting a possible classification as a late-type spiral or an irregular galaxy. The galaxy exhibits a relatively smooth light distribution, but there is some indication of faint spiral arm structure. There is a slight hint of bluer light, perhaps indicative of more recent star formation. The galaxy's overall color suggests a modest stellar population, not dominated by old, red stars. The disk appears slightly warped or disturbed, as the edges are not sharp and the distribution of light does not seem symmetric. There might be a sign of a tidal tail extending from one edge of the galaxy, perhaps due to a past or ongoing interaction with another galaxy. Further spectroscopic analysis is required to confirm this.