The galaxy presents an elongated, cigar-like morphology. It appears largely smooth in texture. The central region exhibits a concentrated brightness, suggesting a bulge. The color profile is dominated by redder hues, particularly towards the central bulge, possibly indicating an older stellar population or significant dust obscuration. Fainter bluer regions are visible, potentially indicating areas of active star formation, though these are limited. There is no obvious spiral structure apparent. There are no obvious signs of recent major mergers or interactions. There may be a minor distortion of the galaxy’s shape, but further examination would be required to determine if it is in fact a minor disturbance.
