The galaxy presents as a moderately luminous, moderately sized object exhibiting a slightly elongated, cigar-like morphology. It appears primarily smooth in structure, with a subtle central concentration of light. There is a hint of disk-like feature, although it is not sharply defined. The galaxy is approximately 4 kiloparsecs across. Based on the color profile, the galaxy exhibits a redder color, indicative of an older stellar population. It does not display prominent spiral arms or active star-forming regions. There are no signs of a major ongoing merger, although the overall irregular shape cannot exclude minor tidal interactions. The estimated star formation rate is low, and the mass of the galaxy is approximately 10^11 solar masses. The object's redshift of approximately 0.23 suggests that it is relatively distant.