The galaxy presents as an elongated structure, significantly longer than it is wide. A distinct central bulge is visible, exhibiting a yellowish-orange hue indicative of an older stellar population. Extending from this bulge are less defined, fainter arms or extensions, particularly prominent on one side. These extensions appear bluer in color, suggesting the presence of younger, hotter stars and possibly active star formation regions. The galaxy's overall form hints at a possible disruption or interaction, as the structure is not entirely symmetrical. There may be an ongoing or recent merger event which is causing the elongation in the disk shape. A possible tidal tail is observed stemming from the galaxy.
