The galaxy appears to be an elongated, cigar-shaped system, with a smooth overall appearance. The central region exhibits a concentration of light, suggesting a possible bulge or core structure. The galaxy's color profile indicates a mixture of stellar populations, with a generally redder hue dominating, though there are hints of bluer regions, particularly towards the outer edges. These bluer regions may indicate areas of more recent star formation, while the redder areas suggest older, more evolved stars. There is no apparent strong spiral arm structure or distinct dust lanes visible in this image. The galaxy appears relatively isolated, without any obvious signs of ongoing major merger activity or significant tidal distortions. However, a slight asymmetry or faint feature extending from one end cannot be ruled out pending further investigation. The overall impression is of an evolved galaxy, possibly a lenticular or elliptical type, with a moderate amount of star formation activity.
