The galaxy presents as a slightly elongated, cigar-shaped structure. Its light profile appears relatively smooth, without prominent spiral arms or distinct features. The core region displays a higher concentration of light, with the overall color suggesting a bias towards older stellar populations, potentially indicating reduced star formation activity. There are subtle color variations within the galaxy, but the lack of well-defined structures suggests an elliptical or lenticular morphological type. Weak tidal features may indicate a past or ongoing minor interaction.
