The galaxy presents a notable elliptical morphology, appearing cigar-shaped along its major axis. A prominent bulge is observed, exhibiting a yellowish-red hue, suggesting an older stellar population with a relative paucity of ongoing star formation in that region. A flattened disk component is visible, oriented approximately perpendicular to the line of sight. This disk appears bluer in color, indicative of younger, hotter stars and potential star-forming regions. There appear to be no significant signs of interaction or recent merger events, such as tidal tails or heavily distorted morphology. The galaxy appears relatively smooth, with no prominent spiral arm structure or distinct dust lanes readily visible. The estimated size is a radius of approximately 6.6 kpc, and its redshift is estimated to be around 0.12, indicating a considerable distance. Overall, it appears to be a relatively massive galaxy with moderate ongoing star formation, primarily concentrated in its disk component.
