This galaxy exhibits a morphology consistent with an interacting system, potentially a merger in progress. The primary galactic body appears elongated, displaying a cigar-like shape. A significant portion of the visible light emanates from a concentrated central region, suggesting a dense stellar population or active galactic nucleus. The galaxy shows signs of tidal distortion, with faint extensions and asymmetries in its outer regions, indicative of gravitational interactions. Patches of bluer light, interspersed within the galaxy's structure, may denote regions of ongoing star formation. The overall color gradient suggests a mix of stellar populations with some redder regions that may be older, more evolved stars, or dust obscuration.
