The galaxy appears as a moderately luminous, elongated structure. It exhibits a generally smooth morphology with a central concentration of light. The overall shape is somewhat irregular, presenting hints of a possible tidal disturbance or ongoing interaction, although a definitive classification is challenging based on the available image resolution. The galaxy displays a range of colors, primarily concentrated toward redder wavelengths. This suggests a stellar population that is dominated by older stars, potentially indicating relatively low ongoing star formation. However, some bluer patches can be discerned, which might indicate some pockets of more recent star formation. The galaxy’s overall luminosity suggests that it is a relatively massive system.
