The galaxy presents an elongated, cigar-like morphology. Its light distribution appears relatively smooth, with a slightly brighter, somewhat concentrated central region. There is no obvious spiral structure or distinct features, such as prominent dust lanes or knots of star formation. The color seems to be relatively uniform across the galaxy, with a slightly redder hue, suggesting an older stellar population and a lack of significant ongoing star formation. There are no signs of significant tidal disturbances or interactions with other galaxies.
