The galaxy presents a somewhat elongated morphology. It appears primarily smooth in structure, showing little evidence of spiral arms or distinct features. The light distribution suggests a central bulge that gradually fades toward the edges. The color profile indicates a general population of older stars, with a hint of bluer light suggesting some star forming regions within the galaxy. There may be ongoing, but low star formation activity. There is no evidence of a strong tidal interaction or merger event. Its overall shape is cigar-shaped with no significant features.