The galaxy appears as an elongated, moderately luminous structure with a discernible central bulge. A disk component is present but not sharply defined, exhibiting a relatively smooth texture, with only hints of spiral arm structure or other distinct features. The shape is more cigar-shaped than rounded. The galaxy displays a blueish hue overall, likely indicative of ongoing or recent star formation. It has some notable irregularities, but not a very high level of disturbance. The galaxy shows a distribution of stellar populations of both young stars (blue) and older stars (redder in color). The galaxy does not appear to be undergoing a major merger, although there is some evidence of minor interactions or tidal features.