The galaxy presents as a spiral type with a relatively high degree of inclination. Two spiral arms are distinctly visible, exhibiting a medium winding pattern. A prominent bulge is apparent, with a moderate size relative to the overall galaxy disk. There is evidence of a bar structure traversing the central region, although its classification as strong or weak would require a higher resolution image. The galaxy appears undisturbed with no evidence of any significant interactions or merging events with other galaxies. The color profile suggests a mix of stellar populations. A brighter, yellower central bulge indicates the presence of older, redder stars, while the bluer hue in the disk region hints at ongoing star formation within the spiral arms.