The galaxy presents as a roughly elliptical, cigar-shaped structure. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. A colour gradient is visible, transitioning from a yellower core to redder hues in the outer regions. The smooth light distribution in the core implies an older stellar population, while the slight redness in the outer regions may be due to dust absorption or the presence of cooler, older stars. No distinct spiral arms or prominent dust lanes are discernible. A possible galactic interaction or merger is hinted at by a small, diffuse structure in proximity to the main galaxy body. The galaxy shows no distinct signs of active star formation and appears relatively quiescent.
