The galaxy exhibits a defined structure, appearing somewhat irregular in shape. The central region displays a bright, concentrated luminosity, suggesting a dense stellar population or active galactic nucleus. The overall color profile leans towards bluer wavelengths, particularly within the core and the surrounding halo. This may indicate ongoing star formation, with the presence of young, hot stars emitting strongly in the blue portion of the spectrum. Evident are some disturbances in its form and morphology suggesting potentially a minor interaction. It does not exhibit any classic spiral arms. Some light and features emanate from around it. The outer halo of the galaxy appears less distinct. The galaxy appears somewhat compact, with an apparent moderate angular size.
