The galaxy presents an elongated, cigar-shaped morphology. It exhibits a bright, concentrated central bulge or core, characterized by a yellowish-orange hue, suggesting an older stellar population. Extending outward from this central region, there are faint, bluish-tinged features that possibly indicate regions of ongoing star formation. These fainter regions appear somewhat irregular and are asymmetrically distributed, with a more prominent extension towards the upper portion of the image. There is no clear evidence of a well-defined disk structure. The galaxy appears relatively isolated, showing no signs of a major merger event or strong tidal interactions with nearby galaxies within the immediate field of view. The overall smoothness of the light distribution suggests that it could be classified as an early-type spiral or a lenticular galaxy.
