The galaxy presents as an elliptical shape, significantly elongated and appearing almost cigar-shaped when viewed from our perspective. The galaxy exhibits a relatively smooth texture, suggesting a lack of prominent spiral arms or significant dust lanes. There is an apparent lack of intricate details, pointing to an older stellar population that could be in the process of fading or has already faded. The colors appear relatively uniform throughout the galaxy, with a slightly redder hue, indicating that it is composed mainly of older stars with lower star formation rates. There are no obvious indications of a strong tidal disturbance or major merger, though minor disturbances cannot be entirely ruled out due to the resolution and depth of the image. Given these characteristics, it is likely a passively evolving galaxy nearing the end of its star-forming activity.
