The galaxy presents an elongated, cigar-like morphology. Its light distribution is dominated by a smooth, centrally concentrated bulge, suggesting a relatively old stellar population with limited ongoing star formation. The color index, trending towards redder hues, supports this assessment.  The galaxy's structure appears largely undisturbed, with no obvious signs of major mergers or significant tidal interactions. However, there is an appearance of a possible tidal tail or a minor disturbance on one end of the galaxy.
